@article {691573,
	title = {The Per-Tau Shell: A Giant Star-forming Spherical Shell Revealed by 3D Dust Observations},
	journal = {The Astrophysical Journal Letters},
	volume = {919},
	number = {1},
	year = {2021},
	pages = {L5},
	abstract = {A major question in the field of star formation is how molecular clouds form out of the diffuse interstellar medium (ISM). Recent advances in 3D dust mapping are revolutionizing our view of the structure of the ISM. Using the highest-resolution 3D dust map to date, we explore the structure of a nearby star-forming region, which includes the well-known Perseus and Taurus molecular clouds. We reveal an extended near-spherical shell, 156 pc in diameter (hereafter called the {\textquotedblleft}Per-Tau Shell{\textquotedblright} ), in which the Perseus and Taurus clouds are embedded. We also find a large ring structure at the location of Taurus (hereafter called the {\textquotedblleft}Tau Ring{\textquotedblright} ). We discuss a formation scenario for the Per-Tau Shell, in which previous stellar and supernova feedback events formed a large expanding shell, where the swept-up ISM has condensed to form both the shell and the Perseus and Taurus molecular clouds within it. We present auxiliary observations of H I,Hα, 26 Al, and X-rays that further support this scenario, and estimate the Per-Tau Shell{\textquoteright}s age to be ≈ 6{\textendash}22 Myrs. The Per-Tau shell offers the first 3D observational view of a phenomenon long-hypothesized theoretically, molecular cloud formation and star formation triggered by previous stellar and supernova feedback.},
	url = {https://doi.org/10.3847/2041-8213/ac1f95},
	author = {Shmuel Bialy and Zucker, Catherine and Goodman, Alyssa A. and Foley, Michael M. and Alves, Jo{\~a}o and Semenov, Vadim A. and Benjamin, Robert and Leike, Reimar and En{\ss}lin, Torsten}
}
@article {691574,
	title = {On the Three-dimensional Structure of Local Molecular Clouds},
	journal = {The Astrophysical Journal},
	volume = {919},
	number = {1},
	year = {2021},
	pages = {35},
	abstract = {We leverage the 1 pc spatial resolution of the Leike et al. three-dimensional (3D)dust map to characterize the 3D structure of nearby molecular clouds (d  400 pc). We start by {\textquotedblleft}skeletonizing{\textquotedblright} the clouds in 3D volume density space to determine their {\textquotedblleft}spines,{\textquotedblright} which we project on the sky to constrain cloud distances with ≈ 1\% uncertainty. For each cloud, we determine an average radial volume density profile around its 3D spine and fit the profiles using Gaussian and Plummer functions. The radial volume density profiles are well described by a two-component Gaussian function, consistent with clouds having broad, lower-density outer envelopes and narrow, higher-density inner layers. The ratio of the outer to inner envelope widths is ≈ 3:1. We hypothesize that these two components may be tracing a transition between atomic and diffuse molecular gas or between the unstable and cold neutral medium. Plummer-like models can also provide a good fit, with molecular clouds exhibiting shallow power-law wings with density, n, falling off like n- 2 at large radii. Using Bayesian model selection, we find that parameterizing the clouds{\textquoteright} profiles using a single Gaussian is disfavored. We compare our results with two- dimensional dust extinction maps, finding that the 3D dust recovers the total cloud mass from integrated approaches with fidelity, deviating only at higher levels of extinction (AV  2{\textendash}3 mag). The 3D cloud structure described here will enable comparisons with synthetic clouds generated in simulations, offering unprecedented insight into the origins and fates of molecular clouds in the interstellar medium.},
	url = {https://doi.org/10.3847/1538-4357/ac1f96},
	author = {Zucker, Catherine and Goodman, Alyssa A. and Alves, Jo{\~a}o and Shmuel Bialy and Koch, Eric W. and Speagle, Joshua S. and Foley, Michael M. and Finkbeiner, Douglas and Leike, Reimar and En{\ss}lin, Torsten and Peek, Joshua E.G. and Edenhofer, Gordian}
}
@article {670931,
	title = {The CARMA-NRO Orion Survey: Filament Formation via Collision-induced Magnetic Reconnectionthe Stick in Orion A},
	journal = {The Astrophysical Journal},
	volume = {906},
	year = {2021},
	pages = {80},
	abstract = {A unique filament is identified in the Herschel maps of the Orion A giant molecular cloud. The filament, which we name the Stick, is ruler-straight and at an early evolutionary stage. Transverse position{\textendash}velocity diagrams show two velocity components closing in on the Stick. The filament shows consecutive rings/forks in C18O (1-0) channel maps, which is reminiscent of structures generated by magnetic reconnection. We propose that the Stick formed via collision-induced magnetic reconnection (CMR). We use the magnetohydrodynamics code Athena++ to simulate the collision between two diffuse molecular clumps, each carrying an antiparallel magnetic field. The clump collision produces a narrow, straight, dense filament with a factor of \&gt;200 increase in density. The production of the dense gas is seven times faster than freefall collapse. The dense filament shows ring/fork-like structures in radiative transfer maps. Cores in the filament are confined by surface magnetic pressure. CMR can be an important dense-gas-producing mechanism in the Galaxy and beyond.},
	url = {http://dx.doi.org/10.3847/1538-4357/abc687},
	author = {Kong, Shuo and Ossenkopf-Okada, Volker and Arce, H{\'e}ctor G. and Bally, John and S{\'a}nchez-Monge, {\'A}lvaro and McGehee, Peregrine and S{\"u}meyye Suri and Klessen, Ralf S. and Carpenter, John M. and Lis, Dariusz C. and Nakamura, Fumitaka and Schilke, Peter and Smith, Rowan J. and Mairs, Steve and Goodman, Alyssa and Mar{\'\i}a Jos{\'e} Maureira}
}
@article {670929,
	title = {Evidence for Radial Expansion at the Core of the Orion Complex with Gaia EDR3},
	journal = {arXiv},
	volume = {2101},
	number = {10380},
	year = {2021},
	abstract = {We present a phase-space study of two stellar groups located at the core of the Orion complex: Brice{\~n}o-1 and Orion Belt Population-near (OBP-near). We identify the groups with the unsupervised clustering algorithm, Shared Nearest Neighbor (SNN), which previously identified twelve new stellar substructures in the Orion complex. For each of the two groups, we derive the 3D space motions of individual stars using Gaia EDR3 proper motions supplemented by radial velocities from Gaia DR2, APOGEE-2, and GALAH DR3. We present evidence for radial expansion of the two groups from a common center. Unlike previous work, our study suggests that evidence of stellar group expansion is confined only to OBP-near and Brice{\~n}o-1 whereas the rest of the groups in the complex show more complicated motions. Interestingly, the stars in the two groups lie at the center of a dust shell, as revealed via an extant 3D dust map. The exact mechanism that produces such coherent motions remains unclear, while the observed radial expansion and dust shell suggest that massive stellar feedback could have influenced the star formation history of these groups.},
	author = {Cameren Swiggum and Elena D{\textquoteright}Onghia and Alves, Jo{\~a}o and Gro{\ss}schedl, Josefa and Michael Foley and Zucker, Catherine and Meingast, Stefan and Boquan Chen and Goodman, Alyssa}
}
@article {670930,
	title = {Dissecting the super-critical filaments embedded in the 0.5 pc subsonic region of Barnard 5},
	journal = {arXiv},
	volume = {2101},
	number = {00248},
	year = {2021},
	abstract = {We characterize in detail the two ~0.3 pc long filamentary structures found within the subsonic region of Barnard 5. We use combined GBT and VLA observations of the molecular lines NH3(1,1) and (2,2) at a resolution of 1800 au, as well as JCMT continuum observations at 850 and 450\&nbsp;μm at a resolution of 4400 au and 3000 au, respectively. We find that both filaments are highly super-critical with a mean mass per unit length,\&nbsp;M/L, of ~80 M⊙\&nbsp;pc-1, after background subtraction, with local increases reaching values of ~150 M⊙\&nbsp;pc-1. This would require a magnetic field strength of ~500\&nbsp;μG to be stable against radial collapse.We extract equidistant cuts perpendicular to the spine of the filament and fit a modified Plummer profile as well as a Gaussian to each of the cuts. The filament widths (deconvolved FWHM) range between 6500-7000 au (~0.03 pc) along the filaments. This equals ~2.0 times the radius of the flat inner region. We find an anti-correlation between the central density and this flattening radius, suggestive of contraction. Further, we also find a strong correlation between the power-law exponent at large radii and the flattening radius. We note that the measurements of these three parameters fall in a plane and derive their empirical relation. Our high-resolution observations provide direct constraints of the distribution of the dense gas within super-critical filaments showing pre- and protostellar activity.},
	url = {https://arxiv.org/abs/2101.00248},
	author = {Schmiedeke, Anika and Pineda, Jaime E. and Caselli, Paola and Arce, H{\'e}ctor G. and Gary A Fuller and Goodman, Alyssa A. and Mar{\'\i}a Jos{\'e} Maureira and Stella S. R. Offner and Segura-Cox, Dominique and Daniel Seifried}
}
@article {670928,
	title = {The \(\rho\) Oph region revisited with Gaia EDR3},
	journal = {arXiv},
	volume = {2101},
	number = {12200},
	year = {2021},
	abstract = {Context. Young and embedded stellar populations are important probes of the star formation process. Paradoxically, we have a better census of nearby embedded young populations than the slightly more evolved optically visible young populations. The high accuracy measurements and all-sky coverage of Gaia data are about to change this situation. Aims. This work aims to construct the most complete sample to date of YSOs in the\&nbsp;ρ\&nbsp;Oph region. Methods. We compile a catalog of 761 Ophiuchus YSOs from the literature and crossmatch it with the Gaia EDR3, Gaia-ESO and APOGEE-2 surveys. We apply a multivariate classification algorithm to this catalog to identify new, co-moving population candidates. Results. We find 173 new YSO candidates in the Gaia EDR3 catalog belonging to the\&nbsp;ρ\&nbsp;Oph region. The new sources appear to be mainly Class III M-stars and substellar objects and are less extincted than the known members. We find 19 previously unknown sources with disks. The analysis of the proper motion distribution of the entire sample reveals a well-defined bimodality, implying two distinct populations sharing a similar 3D volume. The first population comprises young stars{\textquoteright} clusters around the\&nbsp;ρ\&nbsp;Ophiuchi star and the main Ophiuchus clouds (L1688, L1689, L1709). In contrast, the second population is older (\~{}\&nbsp;10 Myr), dispersed, has a distinct proper motion, and is likely part of the Upper-Sco group. The two populations are moving away from each other at about 3.8 km/s, and will no longer overlap in about 4 Myr. Finally, we flag 47 sources in the literature as impostors, which are sources that exhibit large deviations from the average distance and proper motion properties of the\&nbsp;ρ\&nbsp;Oph population. Our results show the importance of accurate 3D space and motion information for improved stellar population analysis.},
	author = {Natalie Grasser and Sebastian Ratzenb{\"o}ck and Alves, Jo{\~a}o and Gro{\ss}schedl, Josefa and Meingast, Stefan and Zucker, Catherine and Hacar, Alvaro and Lada, Charles and Goodman, Alyssa and Lombardi, Marco and John C. Forbes and Immanuel M. Bomze and Torsten M{\"o}ller}
}
@article {662810,
	title = {A Compendium of Distances to Molecular Clouds in the Star Formation Handbook},
	journal = {Astronomy and Astrophysics},
	volume = {633},
	year = {2020},
	pages = {A51},
	abstract = {Accurate distances to local molecular clouds are critical for understanding the star and planet formation process, yet distance measurements are often obtained inhomogeneously on a cloud-by-cloud basis. We have recently developed a method that combines stellar photometric data with Gaia DR2 parallax measurements in a Bayesian framework to infer the distances of nearby dust clouds to a typical accuracy of \~{}5\%. After refining the technique to target lower latitudes and incorporating deep optical data from DECam in the southern Galactic plane, we have derived a catalog of distances to molecular clouds in Reipurth (2008, Star Formation Handbook, Vols. I and II) which contains a large fraction of the molecular material in the solar neighborhood. Comparison with distances derived from maser parallax measurements towards the same clouds shows our method produces consistent distances with ≲10\% scatter for clouds across our entire distance spectrum (150 pc-2.5 kpc). We hope this catalog of homogeneous distances will serve as a baseline for future work. Table A.1 is also available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz- bin/cat/J/A+A/633/A51. It is also available on the Harvard Dataverse at http://https://doi.org/1 0.7910/DVN/07L7YZ An interactive 3D version of Fig. 2 is available at http://https://www.aanda.org},
	author = {Zucker, Catherine and Speagle, Joshua S. and Schlafly, Edward F. and Green, Gregory M. and Finkbeiner, Douglas P. and Goodman, Alyssa and Alves, Jo{\~a}o}
}
@article {670925,
	title = {Core Formation, Coherence and Collapse: A New Core Evolution Paradigm Revealed by Machine Learning},
	journal = {arXiv},
	number = {2006},
	year = {2020},
	pages = {07325},
	abstract = {We study the formation, evolution and collapse of dense cores by tracking density structures in a magnetohydrodynamic (MHD) simulation. We identify cores using the dendrogram algorithm and utilize machine learning techniques, including principal component analysis (PCA) and the k-means clustering algorithm to analyze the full density and velocity dispersion profiles of these cores. We find that there exists an evolutionary sequence consisting of three distinct phases: i) the formation of turbulent density structures (Phase I), ii) the dissipation of turbulence and the formation of coherent cores (Phase II), and iii) the transition to protostellar cores through gravitational collapse (Phase III). In dynamically evolving molecular clouds, the existence of these three phases corresponds to the coexistence of three populations of cores with distinct physical properties. The prestellar and protostellar cores frequently analyzed in previous studies of observations and simulations belong to the last phase in this evolutionary picture. We derive typical lifetimes of 1.4{\textpm}1.0{\texttimes}105\&nbsp;yr, 3.3{\textpm}1.4{\texttimes}105\&nbsp;yr and 3.3{\textpm}1.4{\texttimes}105\&nbsp;yr, respectively for Phase I, II and III. We find that cores can form from both converging flows and filament fragmentation and that cores may form both inside and outside the filaments. We then compare our results to previous observations of coherent cores and provide suggestions for future observations to study cores belonging to the three phases.},
	author = {How-Huan Chen, Hope and Stella S. R. Offner and Pineda, Jaime E. and Goodman, Alyssa A. and Burkert, Andreas and Ginsburg, Adam and Spandan Choudhury}
}
@article {670926,
	title = {Efficient Methanol Production on the Dark Side of a Prestellar Core},
	journal = {The Astrophysical Journal},
	volume = {895},
	year = {2020},
	pages = {101},
	abstract = {We present Atacama Large Millimeter/submillimeter Array maps of the starless molecular cloud core Ophiuchus/H-MM1 in the lines of deuterated ammonia (ortho-), methanol (), and sulfur monoxide (SO). The dense core is seen in\&nbsp;\&nbsp;emission, whereas the\&nbsp;\&nbsp;and SO distributions form a halo surrounding the core. Because methanol is formed on grain surfaces, its emission highlights regions where desorption from grains is particularly efficient. Methanol and sulfur monoxide are most abundant in a narrow zone that follows the eastern side of the core. This side is sheltered from the stronger external radiation field coming from the west. We show that photodissociation on the illuminated side can give rise to an asymmetric methanol distribution but that the stark contrast observed in H-MM1 is hard to explain without assuming enhanced desorption on the shaded side. The region of the brightest emission has a wavy structure that rolls up at one end. This is the signature of Kelvin{\textendash}Helmholtz instability occurring in sheared flows. We suggest that in this zone, methanol and sulfur are released as a result of grain{\textendash}grain collisions induced by shear vorticity.},
	author = {Jorma Harju and Pineda, Jaime E. and Anton I. Vasyunin and Caselli, Paola and Stella S. R. Offner and Goodman, Alyssa A.}
}
@article {670920,
	title = {Ubiquitous NH\(_{3}\) supersonic component in L1688 coherent cores},
	journal = {A\&A},
	volume = {640},
	year = {2020},
	pages = {L6},
	abstract = {
	Context.\&nbsp;Star formation takes place in cold dense cores in molecular clouds. Earlier observations have found that dense cores exhibit subsonic non-thermal velocity dispersions. In contrast, CO observations show that the ambient large-scale cloud is warmer and has supersonic velocity dispersions.



	Aims.\&nbsp;We aim to study the ammonia (NH3) molecular line profiles with exquisite sensitivity towards the coherent cores in L1688 in order to study their kinematical properties in unprecedented detail.



	Methods.\&nbsp;We used NH3\&nbsp;(1,1) and (2,2) data from the first data release (DR1) in the Green Bank Ammonia Survey (GAS). We first smoothed the data to a larger beam of 1' to obtain substantially more extended maps of velocity dispersion and kinetic temperature, compared to the DR1 maps. We then identified the coherent cores in the cloud and analysed the averaged line profiles towards the cores.



	Results.\&nbsp;For the first time, we detected a faint (mean NH3(1,1) peak brightness \&lt; 0.25 K in\&nbsp;TMB), supersonic component towards all the coherent cores in L1688. We fitted two components, one broad and one narrow, and derived the kinetic temperature and velocity dispersion of each component. The broad components towards all cores have supersonic linewidths (ℳS >= 1). This component biases the estimate of the narrow dense core component{\textquoteright}s velocity dispersion by ≈28\% and the kinetic temperature by ≈10\%, on average, as compared to the results from single-component fits.



	Conclusions.\&nbsp;Neglecting this ubiquitous presence of a broad component towards all coherent cores causes the typical single-component fit to overestimate the temperature and velocity dispersion. This affects the derived detailed physical structure and stability of the cores estimated from NH3\&nbsp;observations.

},
	url = {https://doi.org/10.1051/0004-6361/202037955},
	author = {Spandan Choudhury and Pineda, Jaime E. and Caselli, Paola and Ginsburg, Adam and Stella S. R. Offner and Rosolowsky, Erik and Friesen, Rachel K. and Alves, Felipe O. and Chac{\'o}n-Tanarro, Ana and Punanova, Anna and Redaelli, Elena and Helen Kirk, Philip and C. Myers and Peter G. Martin and Shirley, Yancy and Chun-Yuan Chen, Michael and Goodman, Alyssa A. and Di Francesco, James}
}
@article {670918,
	title = {Constraining the distance to the North Polar Spur with Gaia DR2},
	journal = {MNRAS},
	number = {498},
	year = {2020},
	pages = {5863-5872},
	abstract = {The North Polar Spur (NPS) is one of the largest structures observed in the Milky Way in both the radio and soft X-rays. While several predictions have been made regarding the origin of the NPS, modelling the structure is difficult without precise distance constraints. In this paper, we determine accurate distances to the southern terminus of the NPS and towards latitudes ranging up to 55{\textdegree}. First, we fit for the distance and extinction to stars towards the NPS using optical and near-infrared photometry and\&nbsp;Gaia\&nbsp;Data Release 2 astrometry. We model these per-star distance{\textendash}extinction estimates as being caused by dust screens at unknown distances, which we fit for using a nested sampling algorithm. We then compare the extinction to the Spur derived from our 3D dust modelling with integrated independent measures from\&nbsp;XMM{\textendash}Newton\&nbsp;X-ray absorption and H I\&nbsp;column density measures. We find that we can account for nearly 100\&nbsp;per cent of the total column density of the NPS as lying within 140\&nbsp;pc for latitudes \&gt;26{\textdegree} and within 700\&nbsp;pc for latitudes \&lt;11{\textdegree}. Based on the results, we conclude that the NPS is not associated with the Galactic Centre or the Fermi bubbles. Instead, it is likely associated, especially at higher latitudes, with the Scorpius{\textendash}Centaurus association.},
	author = {Kaustav K. Das and Zucker, Catherine and Speagle, Joshua S. and Goodman, Alyssa and Green, Gregory M. and Alves, Jo{\~a}o}
}
@article {662649,
	title = {A Galactic-Scale Gas Wave in the Solar Neighbourhood},
	journal = {Nature},
	volume = {578},
	year = {2020},
	pages = {237{\textendash}239},
	abstract = {For the past 150 years, the prevailing view of the local interstellar medium has been based on a peculiarity known as the Gould Belt1-4, an expanding ring of young stars, gas and dust, tilted about 20 degrees to the Galactic plane. However, the physical relationship between local gas clouds has remained unknown because the accuracy in distance measurements to such clouds is of the same order as, or larger than, their sizes5-7. With the advent of large photometric surveys8 and the astrometric survey9, this situation has changed10. Here we reveal the three- dimensional structure of all local cloud complexes. We find a narrow and coherent 2.7-kiloparsec arrangement of dense gas in the solar neighbourhood that contains many of the clouds thought to be associated with the Gould Belt. This finding is inconsistent with the notion that these clouds are part of a ring, bringing the Gould Belt model into question. The structure comprises the majority of nearby star-forming regions, has an aspect ratio of about 1:20 and contains about three million solar masses of gas. Remarkably, this structure appears to be undulating, and its three-dimensional shape is well described by a damped sinusoidal wave on the plane of the Milky Way with an average period of about 2 kiloparsecs and a maximum amplitude of about 160 parsecs.},
	url = {https://doi.org/10.1038/s41586-019-1874-z},
	author = {Alves, Jo{\~a}o and Zucker, Catherine and Goodman, Alyssa A. and Speagle, Joshua S. and Meingast, Stefan and Robitaille, Thomas and Finkbeiner, Douglas P. and Schlafly, Edward F. and Green, Gregory M.}
}
@article {670919,
	title = {A Prospective ISRO-CfA Himalayan Sub-millimeter-wave Observatory Initiative},
	journal = {arXiv},
	volume = {2008},
	number = {07453},
	year = {2020},
	abstract = {The Smithsonian Astrophysical Observatory (SAO), a member of the Center for Astrophysics | Harvard and Smithsonian, is in discussions with the Space Applications Centre (SAC) of the Indian Space Research Organization (ISRO) and its partners in the newly formed Indian Sub-millimetre-wave Astronomy Alliance (ISAA), to collaborate in the construction of a sub-millimeter-wave astronomy observatory in the high altitude deserts of the Himalayas, initially at the 4500 m Indian Astronomical Observatory, Hanle. Two primary science goals are targeted. One is the mapping of the distribution of neutral atomic carbon, and the carbon monoxide (CO) molecule in higher energy states, in large parts of the Milky Way, and in selected external galaxies. Such studies would advance our understanding of molecular hydrogen present in the interstellar medium, but partly missed by existing observations; and characterize Galaxy-wide molecular cloud excitation conditions, through multi-level CO observations. Stars form in interstellar clouds of molecular gas and dust, and these observations would allow research into the formation and destruction processes of such molecular clouds and the life cycle of galaxies. As the second goal, the observatory would add a new location to the global Event Horizon Telescope (EHT) network, which lacks a station in the Himalayan longitudes. This addition would enhance the quality of the images synthesized by the EHT, support observations in higher sub-millimeter wave bands, sharpening its resolving ability, improve its dynamic imaging capability and add weather resilience to observing campaigns. In the broader context, this collaboration can be a starting point for a wider, mutually beneficial scientific exchange between the Indian and US astronomy communities, including a potential future EHT space component.},
	url = {https://arxiv.org/abs/2008.07453},
	author = {T. K. Sridharan and Shmuel Bialy and Raymond Blundell and Andrew Burkhardt and Thomas Dame and Sheperd Doeleman and Finkbeiner, Douglas and Goodman, Alyssa and alia}
}
@article {662805,
	title = {Relative Alignment between Dense Molecular Cores and Ambient Magnetic Field: The Synergy of Numerical Models and Observations},
	journal = {arXiv E-Prints},
	year = {2020},
	abstract = {
	The role played by magnetic field during star formation is an important topic in astrophysics. We investigate the correlation between the orientation of star-forming cores (as defined by the core major axes) and ambient magnetic field directions in 1) a 3D MHD simulation, 2) synthetic observations generated from the simulation at different viewing angles, and 3) observations of nearby molecular clouds. We find that the results on relative alignment between cores and background magnetic field in synthetic observations slightly disagree with those measured in fully 3D simulation data, which is partly because cores identified in projected 2D maps tend to coexist within filamentary structures, while 3D cores are generally more rounded. In addition, we examine the progression of magnetic field from pc- to core-scale in the simulation, which is consistent with the anisotropic core formation model that gas preferably flow along the magnetic field toward dense cores. When comparing the observed cores identified from the GBT Ammonia Survey (GAS) and Planck polarization-inferred magnetic field orientations, we find that the relative core-field alignment has a regional dependence among different clouds. More specifically, we find that dense cores in the Taurus molecular cloud tend to align perpendicular to the background magnetic field, while those in Perseus and Ophiuchus tend to have random (Perseus) or slightly parallel (Ophiuchus) orientations with respect to the field. We argue that this feature of relative core-field orientation could be used to probe the relative significance of the magnetic field within the cloud.

},
	author = {Chen, Che-Yu and Erica A. Behrens and Jasmin E. Washington and Fissel, Laura M. and Friesen, Rachel K. and Li, Zhi-Yun and Pineda, Jaime E. and alia}
}
@article {663021,
	title = {Droplets. II. Internal Velocity Structures and Potential Rotational Motions in Pressure-Dominated Coherent Structures},
	journal = {The Astrophysical Journal},
	volume = {886},
	year = {2019},
	pages = {119},
	abstract = {We present an analysis of the internal velocity structures of the newly identified sub-0.1 pc coherent structures, droplets, in L1688 and B18. By fitting 2D linear velocity fields to the observed maps of velocity centroids, we determine the magnitudes of linear velocity gradients and examine the potential rotational motions that could lead to the observed velocity gradients. The results show that the droplets follow the same power-law relation between the velocity gradient and size found for larger-scale dense cores. Assuming that rotational motion giving rise to the observed velocity gradient in each core is a solid-body rotation of a rotating body with a uniform density, we derive the {\textquotedblleft}net rotational motions{\textquotedblright} of the droplets. We find a ratio between rotational and gravitational energies, β, of \~{}0.046 for the droplets, and when including both droplets and larger-scale dense cores, we find β \~{} 0.039. We then examine the alignment between the velocity gradient and the major axis of each droplet, using methods adapted from the histogram of relative orientations introduced by Soler et al. We find no definitive correlation between the directions of velocity gradients and the elongations of the cores. Lastly, we discuss physical processes other than rotation that may give rise to the observed velocity field.},
	url = {https://doi.org/10.3847/1538-4357/ab4ce9},
	author = {How-Huan Chen, Hope and Pineda, Jaime E. and Stella S. R. Offner and Goodman, Alyssa A. and Burkert, Andreas and Friesen, Rachel K. and Rosolowsky, Erik and Scibelli, Samantha and Shirley, Yancy}
}
@article {663025,
	title = {Mass Assembly of Stellar Systems and Their Evolution with the SMA (MASSES){\textemdash}Full Data Release},
	journal = {The Astrophysical Journal. Supplement Series},
	volume = {245},
	year = {2019},
	pages = {21},
	abstract = {We present the Mass Assembly of Stellar Systems and their Evolution with the SMA (MASSES) survey, which uses the Submillimeter Array (SMA) interferometer to map the continuum and molecular lines for all 74 known Class 0/I protostellar systems in the Perseus molecular cloud. The primary goal of the survey is to observe an unbiased sample of young protostars in a single molecular cloud so that we can characterize the evolution of protostars. This paper releases the MASSES 1.3 mm data from the subcompact configuration (̃4" or ̃1000 au resolution), which is the SMA{\textquoteright}s most compact array configuration. We release both uv visibility data and imaged data for the spectral lines CO(2-1), 13CO(2-1), C18O(2-1), and N2D+(3-2), as well as for the 1.3 mm continuum. We identify the tracers that are detected toward each source. We also show example images of continuum and CO(2-1) outflows, analyze C18O(2-1) spectra, and present data from the SVS 13 star- forming region. The calculated envelope masses from the continuum show a decreasing trend with bolometric temperature (a proxy for age). Typical C18O(2-1) line widths are 1.45 km s-1, which is higher than the C18O line widths detected toward Perseus filaments and cores. We find that N2D+(3-2) is significantly more likely to be detected toward younger protostars. We show that the protostars in SVS 13 are contained within filamentary structures as traced by C18O(2-1) and N2D+(3-2). We also present the locations of SVS 13A{\textquoteright}s high-velocity (absolute line-of-sight velocities \&gt;150 km s-1) red and blue outflow components. Data can be downloaded from https://da taverse.harvard.edu/dataverse/MASSES.},
	url = {https://doi.org/10.3847/1538-4365/ab5181},
	author = {Stephens, Ian W. and Bourke, Tyler L. and Dunham, Michael M. and Myers, Philip C. and Pokhrel, Riwaj and Tobin, John J. and Arce, H{\'e}ctor G. and et al.}
}
@article {663027,
	title = {Synthetic Large-Scale Galactic Filaments: On Their Formation, Physical Properties, and Resemblance to Observations},
	journal = {The Astrophysical Journal },
	volume = {887},
	year = {2019},
	pages = {186},
	abstract = {Using a population of large-scale filaments extracted from an AREPO simulation of a Milky Way-like galaxy, we seek to understand the extent to which observed large-scale filament properties (with lengths ≳100 pc) can be explained by galactic dynamics alone. From an observer{\textquoteright}s perspective in the disk of the galaxy, we identify filaments forming purely due to galactic dynamics, without the effects of feedback or local self-gravity. We find that large-scale galactic filaments are intrinsically rare, and we estimate that at maximum approximately one filament per kpc2 should be identified in projection, when viewed from the direction of our Sun in the Milky Way. In this idealized scenario, we find filaments in both the arm and interarm regions and hypothesize that the former may be due to gas compression in the spiral potential wells, with the latter due to differential rotation. Using the same analysis pipeline applied previously to observations, we analyze the physical properties of large-scale galactic filaments and quantify their sensitivity to projection effects and galactic environment (i.e., whether they lie in the arm or interarm regions). We find that observed {\textquotedblleft}Giant Molecular Filaments{\textquotedblright} are consistent with being non-self- gravitating structures dominated by galactic dynamics. Straighter, narrower, and denser {\textquotedblleft}Bone-like{\textquotedblright} filaments, like the paradigmatic Nessie filament, have similar column densities, velocity gradients, and galactic plane heights (z ≈ 0 pc) to those in our simple model, but additional physical effects (such as feedback and self-gravity) must be invoked to explain their lengths and widths.},
	url = {https://doi.org/10.3847/1538-4357/ab517d},
	author = {Zucker, Catherine and Rowan Smith and Goodman, Alyssa}
}
@article {663026,
	title = {Visualizing Seasons and Moon Phases with WorldWide Telescope},
	journal = {Advancing Astronomy for All: ASP 2018 ASP Conference Series},
	volume = {524},
	year = {2019},
	pages = {125},
	abstract = {
	WorldWide Telescope (WWT) is a powerful visualization program that allows users to connect Earth-based and space-based views of the Sun- Earth-Moon system. By blending hands-on physical activities with WWT{\textquoteright}s virtual models, students can visualize spatially complex concepts like seasons, Moon phases, and eclipses. In this workshop, we will demonstrate how WWT and the physical models are used together in our WWT ThinkSpace curriculum, developed with funding from the National Science Foundation. We will also present student learning outcomes based on written assessments and student interviews.

},
	url = {https://ui.adsabs.harvard.edu/abs/2019ASPC..524..125U},
	author = {P. Udomprasert and H. Houghton and S. Sunbury and J. Plummer and E. Wright and Goodman, A. and E. Johnson and Zhang, H. and A. Vaishampayan and K. Cho}
}
@article {663020,
	title = {Droplets. I. Pressure-Dominated Coherent Structures in L1688 and B18},
	journal = {The Astrophysical Journal},
	volume = {877},
	year = {2019},
	pages = {93},
	abstract = {We present the observation and analysis of newly discovered coherent structures in the L1688 region of Ophiuchus and the B18 region of Taurus. Using data from the Green Bank Ammonia Survey, we identify regions of high density and near-constant, almost-thermal velocity dispersion. We reveal 18 coherent structures are revealed, 12 in L1688 and 6 in B18, each of which shows a sharp {\textquotedblleft}transition to coherence{\textquotedblright} in velocity dispersion around its periphery. The identification of these structures provides a chance to statistically study the coherent structures in molecular clouds. The identified coherent structures have a typical radius of 0.04 pc and a typical mass of 0.4 M ☉, generally smaller than previously known coherent cores identified by Goodman et al., Caselli et al., and Pineda et al. We call these structures {\textquotedblleft}droplets.{\textquotedblright} We find that, unlike previously known coherent cores, these structures are not virially bound by self-gravity and are instead predominantly confined by ambient pressure. The droplets have density profiles shallower than a critical Bonnor-Ebert sphere, and they have a velocity (V LSR) distribution consistent with the dense gas motions traced by NH3 emission. These results point to a potential formation mechanism through pressure compression and turbulent processes in the dense gas. We present a comparison with a magnetohydrodynamic simulation of a star-forming region, and we speculate on the relationship of droplets with larger, gravitationally bound coherent cores, as well as on the role that droplets and other coherent structures play in the star formation process.},
	url = {https://doi.org/10.3847/1538-4357/ab1a40},
	author = {How-Huan Chen, Hope and Pineda, Jaime E. and Goodman, Alyssa A. and Burkert, Andreas and Stella S. R. Offner and Friesen, Rachel K. and Myers, Philip C. and et al}
}
@article {663022,
	title = {Relative Alignment between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud Using Low- and High-Density Tracers},
	journal = {The Astrophysical Journal },
	volume = {878},
	year = {2019},
	pages = {110},
	abstract = {
	We compare the magnetic field orientation for the young giant molecular cloud Vela C inferred from 500 μm polarization maps made with the BLASTPol balloon-borne polarimeter to the orientation of structures in the integrated line emission maps from Mopra observations. Averaging over the entire cloud we find that elongated structures in integrated line-intensity or zeroth-moment maps, for low-density tracers such as 12CO and 13CO J {\textrightarrow} 1 - 0, are statistically more likely to align parallel to the magnetic field, while intermediate- or high-density tracers show (on average) a tendency for alignment perpendicular to the magnetic field. This observation agrees with previous studies of the change in relative orientation with column density in Vela C, and supports a model where the magnetic field is strong enough to have influenced the formation of dense gas structures within Vela C. The transition from parallel to no preferred/perpendicular orientation appears to occur between the densities traced by 13CO and by C18O J {\textrightarrow} 1 - 0. Using RADEX radiative transfer models to estimate the characteristic number density traced by each molecular line, we find that the transition occurs at a molecular hydrogen number density of approximately 103 cm-3. We also see that the Centre Ridge (the highest column density and most active star-forming region within Vela C) appears to have a transition at a lower number density, suggesting that this may depend on the evolutionary state of the cloud.

},
	url = {https://doi.org/10.3847/1538-4357/ab1eb0},
	author = {Fissel, Laura M. and Peter A. R. Ade and Francesco E. Angil{\`e} and Ashton, Peter and Benton, Steven J. and Che-Yu Che and Cunningham, Maria and et al.}
}
@article {663023,
	title = {The Next Decade of Astroinformatics and Astrostatistics},
	journal = {Bulletin of the American Astronomical Society},
	volume = {51},
	year = {2019},
	pages = {355},
	abstract = {
	Over the past century, major advances in astronomy and astrophysics have been driven by improvements in instrumentation. With the amassing of high quality data from new telescopes it is becoming clear that research in astrostatistics and astroinformatics will be necessary to develop new methodology needed in astronomy.

},
	url = {https://ui.adsabs.harvard.edu/abs/2019BAAS...51c.355S},
	author = {Siemiginowska, Aneta and Gwendolyn Eadie and Ian Czekala and Feigelson, Eric and Eric B. Ford and Kashyap, Vinay and Michael Kuhn and et al.}
}
@article {663024,
	title = {Histogram of Oriented Gradients: A Technique for the Study of Molecular Cloud Formation},
	journal = {Astronomy and Astrophysics},
	volume = {622},
	year = {2019},
	pages = {A166},
	abstract = {
	We introduce the histogram of oriented gradients (HOG), a tool developed for machine vision that we propose as a new metric for the systematic characterization of spectral line observations of atomic and molecular gas and the study of molecular cloud formation models. In essence, the HOG technique takes as input extended spectral-line observations from two tracers and provides an estimate of their spatial correlation across velocity channels. We characterized HOG using synthetic observations of HI and 13CO (J = 1 {\textrightarrow} 0) emission from numerical simulations of magnetohydrodynamic (MHD) turbulence leading to the formation of molecular gas after the collision of two atomic clouds. We found a significant spatial correlation between the two tracers in velocity channels where vHI ≈ v13CO, almost independent of the orientation of the collision with respect to the line of sight. Subsequently, we used HOG to investigate the spatial correlation of the HI, from The HI/OH/recombination line survey of the inner Milky Way (THOR), and the 13CO (J = 1 {\textrightarrow} 0) emission from the Galactic Ring Survey (GRS), toward the portion of the Galactic plane 33{\textdegree}.75 <=l <= 35{\textdegree}.25 and |b| <= 1{\textdegree}.25. We found a significant spatial correlation between the two tracers in extended portions of the studied region. Although some of the regions with high spatial correlation are associated with HI self-absorption (HISA) features, suggesting that it is produced by the cold atomic gas, the correlation is not exclusive to this kind of region. The HOG results derived for the observational data indicate significant differences between individual regions: some show spatial correlation in channels around vHI ≈ v13CO while others present spatial correlations in velocity channels separated by a few kilometers per second. We associate these velocity offsets to the effect of feedback and to the presence of physical conditions that are not included in the atomic-cloud-collision simulations, such as more general magnetic field configurations, shear, and global gas infall.

},
	url = {https://doi.org/10.1051/0004-6361/201834300},
	author = {J.D. Soler and Beuther, H. and Rugel, M. and Y. Wang, and P. C. Clark and S. C. O. Glover and P. F. Goldsmith and et al.}
}
@article {670964,
	title = {Cultivating Curiosity with Life in the Universe and WorldWide Telescope},
	journal = { Astronomical Society of the Pacific},
	volume = {524},
	number = {273},
	year = {2019},
	abstract = {When students encounter complex topics like the search for extraterrestrial life, questions abound - thoughtful, unpredictable, and often profound. Despite this thriving curiosity, the first step to be able to explore complex questions is developing the capacity to verbalize a meaningful question. The WorldWide Telescope Ambassadors team designed an out-of-school curriculum called Life in the Universe, which engages middle school-aged students in the science and scientific process of the search for distant life. Students practice generating meaningful questions, which will guide them through the science content, as groups of students build to culminating capstone projects. Results from surveys administered to participating students indicate gains in curiosity in science, as well as in seeing oneself as successful in science.},
	author = {H. Houghton and P. Udomprasert and S. Sunbury and E. Wright and Goodman, A. and E. Johnson and A. Bishop}
}
@article {670972,
	title = {Droplets II: Internal Velocity Structures and Potential Rotational Motions in Coherent Cores},
	journal = {arXiv},
	volume = {1908},
	number = {04367},
	year = {2019},
	abstract = {We present an analysis of the internal velocity structures of the newly identified sub-0.1 pc coherent structures, droplets, in L1688 and B18. By fitting 2D linear velocity fields to the observed maps of velocity centroids, we determine the magnitudes of linear velocity gradients and examine the potential rotational motions that could lead to the observed velocity gradients. The results show that the droplets follow the same power-law relation between the velocity gradient and size found for larger-scale dense cores. Assuming that rotational motion giving rise to the observed velocity gradient in each core is a solid-body rotation of a rotating body with a uniform density, we derive the "net rotational motions" of the droplets. We find a ratio between rotational and gravitational energies,\&nbsp;β, of\&nbsp;\~{}0.046\&nbsp;for the droplets, and when including both droplets and larger-scale dense cores, we find\&nbsp;β\~{}0.039. We then examine the alignment between the velocity gradient and the major axis of each droplet, using methods adapted from the histogram of relative orientations (HRO) introduced by Soler et al. (2013). We find no definitive correlation between the directions of velocity gradients and the elongations of the cores. Lastly, we discuss physical processes other than rotation that may give rise to the observed velocity field.},
	url = {https://arxiv.org/abs/1908.04367},
	author = {How-Huan Chen, Hope and Pineda, Jaime E. and Stella S. R. Offner and Goodman, Alyssa A. and alia}
}
@article {670974,
	title = {Efficient methanol desorption in shear instability},
	journal = {arXiv},
	volume = {1903},
	number = {11298},
	year = {2019},
	abstract = {We present ALMA maps of the starless molecular cloud core Ophiuchus/H-MM1 in the lines of deuterated ammonia (ortho-NH2D), methanol (CH3OH), and sulphur monoxide (SO). The dense core is seen in NH2D emission, whereas the CH3OH and SO distributions form a halo surrounding the core. Because methanol is formed on grain surfaces, its emission highlights regions where desorption from grains is particularly efficient. Methanol and sulphur monoxide are most abundant in a narrow zone that follows the eastern side of the core. This side is sheltered from the stronger external radiation field coming from the west. We show that photodissociation on the illuminated side can give rise to an asymmetric methanol distribution, but that the stark contrast observed in H-MM1 is hard to explain without assuming enhanced desorption on the shaded side. The region of the brightest emission has a wavy structure that rolls up at one end. This is the signature of Kelvin-Helmholtz instability occurring in sheared flows. We suggest that in this zone, methanol and sulphur are released as a result of grain-grain collisions induced by shear vorticity.},
	url = {https://arxiv.org/abs/1903.11298},
	author = {Jorma Harju and Pineda, Jaime E. and Anton I. Vasyunin and Caselli, Paola and Stella S. R. Offner and Goodman, Alyssa A. and alia}
}
@article {2019arXiv190201425Z,
	title = {A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition},
	journal = {arXiv e-prints},
	year = {2019},
	pages = {arXiv:1902.01425},
	keywords = {Astrophysics - Astrophysics of Galaxies},
	author = {Zucker, Catherine and Speagle, Joshua S. and Schlafly, Edward F. and Green, Gregory M. and Finkbeiner, Douglas P. and Goodman, Alyssa A. and Alves, Jo{\~a}o}
}
@article {670966,
	title = {VizieR Online Data Catalog: Distances to molecular clouds in SFR (Zucker+, 2020)},
	journal = {VizieR Online Data Catalog},
	volume = {J/A+A/633/A51},
	year = {2019},
	abstract = {
	Distances to ~60 star-forming regions in Reipurth (2008, Star Formation Handbook, vols I and II) have been computed using stellar photometry and Gaia DR2 parallax measurements. Usually, several distance estimates are taken across each cloud.



	\&nbsp;

For each sightline, the median distance (d50) is provided, plus the 16th and 84th percentiles on the distance probability distribution function. There is an additional systematic uncertainty, which is unknown but estimated to be ~5\% in distance for clouds \&lt;1.5kpc, ~10\% in distance for clouds \&gt;1.5kpc, and ~7\% in distance for the southern clouds Lupus, Chamaeleon, and Corona Australis. These should be added in quadrature with the statistical uncertainties reported in the table. In addition to the distances, ancillary model parameters used in our fit are also included (e.g. the amount of foreground extinction "f"). See Section 3.2.1 and Section 3.2.2 in Zucker et al. (2019ApJ...879..125Z) for a complete description of model parameters.},
	author = {C. Zucker and J. S. Speagle and E. Schlafly and G. M. Green and D. P. Finkbeiner and Goodman, A. and Alves, J.}
}
@article {670971,
	title = {The Role of Machine Learning in the Next Decade of Cosmology},
	journal = {Bulletin of the American Astronomical Society},
	volume = {51},
	number = {14},
	year = {2019},
	abstract = {In recent years, machine learning (ML) methods have remarkably improved how cosmologists can interpret data. The next decade will bring new opportunities for data-driven cosmological discovery, but will also present new challenges for adopting ML methodologies and understanding the results. ML could transform our field, but this transformation will require the astronomy community to both foster and promote interdisciplinary research endeavors.},
	url = {https://arxiv.org/abs/1902.10159},
	author = {Ntampaka, Michelle and Camille Avestruz and Steven Boada and Joao Caldeira and Jessi Cisewski-Kehe and Di Stefano, Rosanne and Dvorkin, Cora and August E. Evrard and Arya Farahi and Finkbeiner, Doug and Genel, Shy and Goodman, Alyssa and alia}
}
@article {2018A\&A...619A.106G,
	title = {3D shape of Orion A from Gaia DR2},
	journal = {Astronomy \& Astrophysics},
	volume = {619},
	year = {2018},
	pages = {A106},
	keywords = {Astrophysics - Astrophysics of Galaxies, local insterstellar matter, methods: observational, Methods: Statistical, parallaxes, stars: distances, stars: formation},
	doi = {10.1051/0004-6361/201833901},
	author = {Gro{\ss}schedl, Josefa E. and Alves, Jo{\~a}o and Meingast, Stefan and Ackerl, Christine and Ascenso, Joana and Bouy, Herv{\'e} and Burkert, Andreas and Forbrich, Jan and F{\"u}rnkranz, Verena and Goodman, Alyssa and Hacar, {\'A}lvaro and Herbst-Kiss, Gabor and Lada, Charles J. and Larreina, Irati and Leschinski, Kieran and Lombardi, Marco and Moitinho, Andr{\'e} and Mortimer, Daniel and Zari, Eleonora}
}
@article {2018ApJS..236...22R,
	title = {AAS WorldWide Telescope: A Seamless, Cross-platform Data Visualization Engine for Astronomy Research, Education, and Democratizing Data},
	journal = {The Astrophysical Journal Supplement Series},
	volume = {236},
	year = {2018},
	pages = {22},
	keywords = {astronomical databases: miscellaneous, Astrophysics - Instrumentation and Methods for Astrophysics, Atlases, Catalogs, surveys, virtual observatory tools},
	doi = {10.3847/1538-4365/aab776},
	author = {Rosenfield, Philip and Fay, Jonathan and Gilchrist, Ronald K. and Cui, Chenzhou and Weigel, A. David and Robitaille, Thomas and Otor, Oderah Justin and Goodman, Alyssa}
}
@article {2018ApJ...859..162C,
	title = {The Anatomy of the Column Density Probability Distribution Function (N-PDF)},
	journal = {The Astrophysical Journal},
	volume = {859},
	year = {2018},
	month = {Jun},
	pages = {162},
	keywords = {Astrophysics - Astrophysics of Galaxies, galaxies: star formation, ISM: clouds, magnetohydrodynamics: MHD},
	doi = {10.3847/1538-4357/aabaf6},
	author = {How-Huan Chen, Hope and Burkhart, Blakesley and Goodman, Alyssa and Collins, David C.}
}
@article {2018ApJS..236...25K,
	title = {The CARMA-NRO Orion Survey},
	journal = {The Astrophysical Journal Supplement Series},
	volume = {236},
	year = {2018},
	pages = {25},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: Jets and Outflows, ISM: Kinematics and Dynamics, ISM: structure, photon-dominated region: PDR, stars: formation},
	doi = {10.3847/1538-4365/aabafc},
	author = {Kong, Shuo and Arce, H{\'e}ctor G. and Feddersen, Jesse R. and Carpenter, John M. and Nakamura, Fumitaka and Shimajiri, Yoshito and Isella, Andrea and Ossenkopf-Okada, Volker and Sargent, Anneila I. and S{\'a}nchez-Monge, {\'A}lvaro and Suri, S{\"u}meyye T. and Kauffmann, Jens and Pillai, Thushara and Pineda, Jaime E. and Koda, Jin and Bally, John and Lis, Dariusz C. and Padoan, Paolo and Klessen, Ralf and Mairs, Steve and Goodman, Alyssa and Goldsmith, Paul and McGehee, Peregrine and Schilke, Peter and Teuben, Peter J. and Jos{\'e} Maureira, Mar{\textquoteright}{\i}a and Hara, Chihomi and Ginsburg, Adam and Burkhart, Blakesley and Smith, Rowan J. and Schmiedeke, Anika and Pineda, Jorge L. and Ishii, Shun and Sasaki, Kazushige and Kawabe, Ryohei and Urasawa, Yumiko and Oyamada, Shuri and Tanabe, Yoshihiro}
}
@article {2018ApJ...861...77M,
	title = {Dense Gas Kinematics and a Narrow Filament in the Orion A OMC1 Region Using NH$_{3}$},
	journal = {The Astrophysical Journal},
	volume = {861},
	year = {2018},
	pages = {77},
	keywords = {astrochemistry, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, ISM: individual objects: OMC1, ISM: Kinematics and Dynamics, ISM: magnetic fields, ISM: molecules, radio lines: ISM},
	doi = {10.3847/1538-4357/aac8da},
	author = {Monsch, Kristina and Pineda, Jaime E. and Liu, Hauyu Baobab and Zucker, Catherine and How-Huan Chen, Hope and Pattle, Kate and Offner, Stella S.~R. and Di Francesco, James and Ginsburg, Adam and Ercolano, Barbara and Arce, H{\'e}ctor G. and Friesen, Rachel and Kirk, Helen and Caselli, Paola and Goodman, Alyssa A.}
}
@article {2018arXiv180910223C,
	title = {Droplets I: Pressure-Dominated Sub-0.1 pc Coherent Structures in L1688 and B18},
	journal = {arXiv e-prints},
	year = {2018},
	pages = {arXiv:1809.10223},
	keywords = {Astrophysics - Astrophysics of Galaxies},
	author = {How-Huan Chen, Hope and Pineda, Jaime E. and Goodman, Alyssa A. and Burkert, Andreas and Offner, Stella S.~R. and Friesen, Rachel K. and Myers, Philip C. and Alves, Felipe and Arce, Hector G. and Caselli, Paola and Chacon-Tanarro, Ana and Chun-Yuan Chen, Michael and Di Francesco, James and Ginsburg, Adam and Keown, Jared and Kirk, Helen and Peter G. Martin and Matzner, Christopher and Punanova, Anna and Redaelli, Elena and Rosolowsky, Erik and Scibelli, Samantha and Seo, Young Min and Shirley, Yancy and Singh, Ayushi}
}
@article {2018arXiv180908338S,
	title = {Histogram of oriented gradients: a technique for the study of molecular cloud formation},
	journal = {arXiv e-prints},
	year = {2018},
	month = {Sep},
	pages = {arXiv:1809.08338},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
	author = {Soler, J.~D. and Beuther, H. and Rugel, M. and Y. Wang, and Clark, P.~C. and Glover, S.~C.~O. and Goldsmith, P.~F. and Heyer, M. and Anderson, L.~D. and Goodman, A. and Henning, Th. and Kainulainen, J. and Klessen, R.~S. and Longmore, S.~N. and McClure-Griffiths, N.~M. and Menten, K.~M. and Mottram, J.~C. and Ott, J. and Ragan, S.~E. and Smith, R.~J. and Urquhart, J.~S. and Bigiel, F. and Hennebelle, P. and Roy, N. and Schilke, P.}
}
@article {2018ApJ...869...83Z,
	title = {Mapping Distances across the Perseus Molecular Cloud Using CO Observations, Stellar Photometry, and Gaia DR2 Parallax Measurements},
	journal = {The Astrophysical Journal},
	volume = {869},
	year = {2018},
	pages = {83},
	keywords = {Astrophysics - Astrophysics of Galaxies, dust, extinction, ISM: clouds, Methods: Statistical},
	doi = {10.3847/1538-4357/aae97c},
	author = {Zucker, Catherine and Schlafly, Edward F. and Speagle, Joshua S. and Green, Gregory M. and Portillo, Stephen K.~N. and Finkbeiner, Douglas P. and Goodman, Alyssa A.}
}
@article {2018ApJS..237...22S,
	title = {Mass Assembly of Stellar Systems and Their Evolution with the SMA (MASSES){\textemdash}1.3 mm Subcompact Data Release},
	journal = {The Astrophysical Journal Supplement Series},
	volume = {237},
	year = {2018},
	pages = {22},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, galaxies: star formation, ISM: clouds, ISM: Jets and Outflows, stars: formation, stars: protostars, surveys},
	doi = {10.3847/1538-4365/aacda9},
	author = {Stephens, Ian W. and Dunham, Michael M. and Myers, Philip C. and Pokhrel, Riwaj and Bourke, Tyler L. and Vorobyov, Eduard I. and Tobin, John J. and Sadavoy, Sarah I. and Pineda, Jaime E. and Offner, Stella S.~R. and Lee, Katherine I. and Kristensen, Lars E. and J{\o}rgensen, Jes K. and Goodman, Alyssa A. and Arce, H{\'e}ctor G. and Gurwell, Mark}
}
@article {2018arXiv180704780A,
	title = {Multi-Messenger Astrophysics: Harnessing the Data Revolution},
	journal = {arXiv e-prints},
	year = {2018},
	pages = {arXiv:1807.04780},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics},
	author = {Allen, Gabrielle and Anderson, Warren and Blaufuss, Erik and Bloom, Joshua S. and Brady, Patrick and Burke-Spolaor, Sarah and Cenko, S. Bradley and Connolly, Andrew and Couvares, Peter and Fox, Derek and Gal-Yam, Avishay and Gezari, Suvi and Goodman, Alyssa and Grant, Darren and Groot, Paul and Guillochon, James and Hanna, Chad and Hogg, David W. and Holley-Bockelmann, Kelly and Howell, D. Andrew and David Kaplan and Katsavounidis, Erik and Kowalski, Marek and Lehner, Luis and Muthukrishna, Daniel and Narayan, Gautham and Peek, J.~E.~G. and Saha, Abhijit and Shawhan, Peter and Taboada, Ignacio}
}
@article {2018arXiv180511300G,
	title = {New Thinking on, and with, Data Visualization},
	journal = {arXiv e-prints},
	year = {2018},
	pages = {arXiv:1805.11300},
	keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	author = {Goodman, Alyssa A. and Michelle A. Borkin and Robitaille, Thomas P.}
}
@article {2018ApJ...864..153Z,
	title = {Physical Properties of Large-scale Galactic Filaments},
	journal = {The Astrophysical Journal},
	volume = {864},
	year = {2018},
	pages = {153},
	keywords = {Astrophysics - Astrophysics of Galaxies, Galaxy: structure, ISM: clouds},
	doi = {10.3847/1538-4357/aacc66},
	author = {Zucker, Catherine and Battersby, Cara and Goodman, Alyssa}
}
@article {2018arXiv180408979F,
	title = {Relative Alignment Between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud using Low and High Density Tracers},
	journal = {arXiv e-prints},
	year = {2018},
	pages = {arXiv:1804.08979},
	keywords = {Astrophysics - Astrophysics of Galaxies},
	author = {Fissel, Laura M. and Ade, Peter A.~R. and ngil{\`e}, Francesco E. and Ashton, Peter and Benton, Steven J. and Chen, Che-Yu and Cunningham, Maria and Devlin, Mark J. and Dober, Bradley and Friesen, Rachel and Fukui, Yasuo and Galitzki, Nicholas and Gandilo, Natalie N. and Goodman, Alyssa and Green, Claire-Elise and Jones, Paul and Klein, Jeffrey and King, Patrick and Korotkov, Andrei L. and Li, Zhi-Yun and Lowe, Vicki and Peter G. Martin and Matthews, Tristan G. and Moncelsi, Lorenzo and Nakamura, Fumitaka and Netterfield, Calvin B. and Newmark, Amanda and Novak, Giles and Pascale, Enzo and Poidevin, Fr{\'e}d{\'e}rick and Santos, Fabio P. and Savini, Giorgio and Scott, Douglas and Shariff, Jamil A. and Diego Soler, Juan and Thomas, Nicholas E. and Tucker, Carole E. and Tucker, Gregory S. and Ward-Thompson, Derek}
}
@article {2017ApJ...846...16S,
	title = {Alignment between Protostellar Outflows and Filamentary Structure},
	journal = {The Astrophysical Journal},
	volume = {846},
	year = {2017},
	month = {Sep},
	pages = {16},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, galaxies: star formation, ISM: clouds, ISM: Jets and Outflows, ISM: structure, stars: formation, stars: protostars},
	doi = {10.3847/1538-4357/aa8262},
	author = {Stephens, Ian W. and Dunham, Michael M. and Myers, Philip C. and Pokhrel, Riwaj and Sadavoy, Sarah I. and Vorobyov, Eduard I. and Tobin, John J. and Pineda, Jaime E. and Offner, Stella S.~R. and Lee, Katherine I. and Kristensen, Lars E. and J{\o}rgensen, Jes K. and Goodman, Alyssa A. and Bourke, Tyler L. and Arce, H{\'e}ctor G. and Plunkett, Adele L.}
}
@article {2017A\&A...605A..58A,
	title = {Galactic supernova remnant candidates discovered by THOR},
	journal = {Astronomy \& Astrophysics},
	volume = {605},
	year = {2017},
	month = {Sep},
	pages = {A58},
	keywords = {Astrophysics - Astrophysics of Galaxies, Hiiregions, infrared: ISM, ISM: supernova remnants, radio continuum: ISM},
	doi = {10.1051/0004-6361/201731019},
	author = {Anderson, L.~D. and Y. Wang, and Bihr, S. and Rugel, M. and Beuther, H. and Bigiel, F. and Churchwell, E. and Glover, S.~C.~O. and Goodman, A.~A. and Henning, Th. and Heyer, M. and Klessen, R.~S. and Linz, H. and Longmore, S.~N. and Menten, K.~M. and Ott, J. and Roy, N. and Soler, J.~D. and Stil, J.~M. and Urquhart, J.~S.}
}
@article {2017ApJ...846..144K,
	title = {The Green Bank Ammonia Survey: Dense Cores under Pressure in Orion A},
	journal = {The Astrophysical Journal},
	volume = {846},
	year = {2017},
	month = {Sep},
	pages = {144},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: Kinematics and Dynamics, radio lines: ISM, stars: formation, submillimeter: ISM},
	doi = {10.3847/1538-4357/aa8631},
	author = {Kirk, Helen and Friesen, Rachel K. and Pineda, Jaime E. and Rosolowsky, Erik and Offner, Stella S.~R. and Matzner, Christopher D. and Myers, Philip C. and Di Francesco, James and Caselli, Paola and Alves, Felipe O. and Chac{\'o}n-Tanarro, Ana and Chen, How-Huan and Chun-Yuan Chen, Michael and Keown, Jared and Punanova, Anna and Seo, Young Min and Shirley, Yancy and Ginsburg, Adam and Hall, Christine and Singh, Ayushi and Arce, H{\'e}ctor G. and Goodman, Alyssa A. and Martin, Peter and Redaelli, Elena}
}
@article {2017ApJ...843...63F,
	title = {The Green Bank Ammonia Survey: First Results of NH$_{3}$ Mapping of the Gould Belt},
	journal = {The Astrophysical Journal},
	volume = {843},
	year = {2017},
	month = {Jul},
	pages = {63},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, B18, ISM: individual objects: L1668, ISM: molecules, NGC1333, OrionA molecular complex, stars: formation},
	doi = {10.3847/1538-4357/aa6d58},
	author = {Friesen, Rachel K. and Pineda, Jaime E. and co-PIs and Rosolowsky, Erik and Alves, Felipe and Chac{\'o}n-Tanarro, Ana and How-Huan Chen, Hope and Chun-Yuan Chen, Michael and Di Francesco, James and Keown, Jared and Kirk, Helen and Punanova, Anna and Seo, Young Min and Shirley, Yancy and Ginsburg, Adam and Hall, Christine and Offner, Stella S.~R. and Singh, Ayushi and Arce, H{\'e}ctor G. and Caselli, Paola and Goodman, Alyssa A. and Peter G. Martin and Matzner, Christopher and Myers, Philip C. and Redaelli, Elena and GAS Collaboration}
}
@article {2017ApJ...850....3K,
	title = {The Green Bank Ammonia Survey: Observations of Hierarchical Dense Gas Structures in Cepheus-L1251},
	journal = {The Astrophysical Journal},
	volume = {850},
	year = {2017},
	month = {Nov},
	pages = {3},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, ISM: Kinematics and Dynamics, ISM: structure, stars: formation},
	doi = {10.3847/1538-4357/aa93ec},
	author = {Keown, Jared and Di Francesco, James and Kirk, Helen and Friesen, Rachel K. and Pineda, Jaime E. and Rosolowsky, Erik and Ginsburg, Adam and Offner, Stella S.~R. and Caselli, Paola and Alves, Felipe and Chac{\'o}n-Tanarro, Ana and Punanova, Anna and Redaelli, Elena and Seo, Young Min and Matzner, Christopher D. and Chun-Yuan Chen, Michael and Goodman, Alyssa A. and Chen, How-Huan and Shirley, Yancy and Singh, Ayushi and Arce, Hector G. and Martin, Peter and Myers, Philip C.}
}
@article {2017PLSCB..13E5399Z,
	title = {Ten simple rules for responsible big data research},
	journal = {PLoS Computational Biology},
	volume = {13},
	year = {2017},
	pages = {e1005399},
	doi = {10.1371/journal.pcbi.1005399},
	author = {Zook, Matthew and Barocas, Solon and boyd, danah and Crawford, Kate and Keller, Emily and Gangadharan, Seeta Pe{\~n}a and Goodman, Alyssa and Hollander, Rachelle and Koenig, Barbara A. and Metcalf, Jacob and Narayanan, Arvind and Alondra Nelson and Pasquale, Frank}
}
@article {2017ApJ...842L...9H,
	title = {Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation},
	journal = {The Astrophysical Journal},
	volume = {842},
	year = {2017},
	month = {Jun},
	pages = {L9},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, ISM: magnetic fields, magnetic fields, magnetohydrodynamics: MHD, polarization, stars: formation, turbulence},
	doi = {10.3847/2041-8213/aa71b7},
	author = {Hull, Charles L.~H. and Mocz, Philip and Burkhart, Blakesley and Goodman, Alyssa A. and Girart, Josep M. and Cort{\'e}s, Paulo C. and Hernquist, Lars and Springel, Volker and Li, Zhi-Yun and Lai, Shih-Ping}
}
@article {2016A\&A...592A..88P,
	title = {First stars of the \ensuremath\rho Ophiuchi dark cloud. XMM-Newton view of \ensuremath\rho Oph and its neighbors},
	journal = {Astronomy \& Astrophysics},
	volume = {592},
	year = {2016},
	month = {Aug},
	pages = {A88},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, open clusters and associations: general, stars: activity, stars: formation, stars: individual: \ensuremath\rhoOphiuchi, X-rays: stars},
	doi = {10.1051/0004-6361/201628284},
	author = {Pillitteri, I. and Wolk, S.~J. and Chen, H.~H. and Goodman, A.}
}
@article {2016MEPS..554..241D,
	title = {Individual variation in seasonal movements and foraging strategies of a land-locked, ice-breeding pinniped},
	journal = {Marine Ecology Progress Series},
	volume = {554},
	year = {2016},
	month = {Jul},
	pages = {241-256},
	doi = {10.3354/meps11804},
	author = {Dmitrieva, L. and J{\"u}ssi, M. and J{\"u}ssi, I. and Kasymbekov, Y. and Verevkin, M. and Baimukanov, M. and Wilson, S. and Goodman}
}
@article {2016ApJ...820L...2L,
	title = {Misalignment of Outflow Axes in the Proto-multiple Systems in Perseus},
	journal = {The Astrophysical Journal},
	volume = {820},
	year = {2016},
	month = {Mar},
	pages = {L2},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, binaries: general, ISM: Kinematics and Dynamics, ISM: molecules, stars: formation, stars: protostars, submillimeter: ISM},
	doi = {10.3847/2041-8205/820/1/L2},
	author = {Lee, Katherine I. and Dunham, Michael M. and Myers, Philip C. and Arce, H{\'e}ctor G. and Bourke, Tyler L. and Goodman, Alyssa A. and J{\o}rgensen, Jes K. and Kristensen, Lars E. and Offner, Stella S.~R. and Pineda, Jaime E. and Tobin, John J. and Vorobyov, Eduard I.}
}
@article {2016ApJ...822...52R,
	title = {A Uniform Catalog of Molecular Clouds in the Milky Way},
	journal = {The Astrophysical Journal},
	volume = {822},
	year = {2016},
	month = {May},
	pages = {52},
	keywords = {Astrophysics - Astrophysics of Galaxies, Galaxy: general, ISM: clouds, ISM: molecules},
	doi = {10.3847/0004-637X/822/1/52},
	author = {Rice, Thomas S. and Goodman, Alyssa A. and Bergin, Edwin A. and Beaumont, Christopher and Dame, T.~M.}
}
@article {2016A\&A...587A.153M,
	title = {VISION - Vienna survey in Orion. I. VISTA Orion A Survey},
	journal = {Astronomy \& Astrophysics},
	volume = {587},
	year = {2016},
	month = {Mar},
	pages = {A153},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, methods: data analysis, stars: formation, stars: pre-main sequence, techniques: image processing},
	doi = {10.1051/0004-6361/201527160},
	author = {Meingast, Stefan and Alves, Jo{\~a}o and Mardones, Diego and Teixeira, Paula Stella and Lombardi, Marco and Gro{\ss}schedl, Josefa and Ascenso, Joana and Bouy, Herve and Forbrich, Jan and Goodman, Alyssa and Hacar, Alvaro and Hasenberger, Birgit and Kainulainen, Jouni and Kubiak, Karolina and Lada, Charles and Lada, Elizabeth and Moitinho, Andr{\'e} and Petr-Gotzens, Monika and Rodrigues, Lara and Rom{\'a}n-Z{\'u}{\~n}iga, Carlos G.}
}
@article {2015Natur.518..213P,
	title = {The formation of a quadruple star system with wide separation},
	journal = {Nature},
	volume = {518},
	year = {2015},
	pages = {213-215},
	doi = {10.1038/nature14166},
	author = {Pineda, Jaime E. and Offner, Stella S.~R. and Parker, Richard J. and Arce, H{\'e}ctor G. and Goodman, Alyssa A. and Caselli, Paola and Fuller, Gary A. and Bourke, Tyler L. and Corder, Stuartt A.}
}
@article {2015ApJ...814..114L,
	title = {Mass Assembly of Stellar Systems and Their Evolution with the SMA (MASSES). Multiplicity and the Physical Environment in L1448N},
	journal = {The Astrophysical Journal},
	volume = {814},
	year = {2015},
	month = {Dec},
	pages = {114},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, binaries: general, ISM: Kinematics and Dynamics, ISM: molecules, stars: formation, stars: protostars, submillimeter: ISM},
	doi = {10.1088/0004-637X/814/2/114},
	author = {Lee, Katherine I. and Dunham, Michael M. and Myers, Philip C. and Tobin, John J. and Kristensen, Lars E. and Pineda, Jaime E. and Vorobyov, Eduard I. and Offner, Stella S.~R. and Arce, H{\'e}ctor G. and Li, Zhi-Yun and Bourke, Tyler L. and J{\o}rgensen, Jes K. and Goodman, Alyssa A. and Sadavoy, Sarah I. and Chandler, Claire J. and Harris, Robert J. and Kratter, Kaitlin and Looney, Leslie W. and Melis, Carl and Perez, Laura M. and Segura-Cox, Dominique}
}
@article {2015ApJ...807..104T,
	title = {Prospects for Chemically Tagging Stars in the Galaxy},
	journal = {The Astrophysical Journal},
	volume = {807},
	year = {2015},
	month = {Jul},
	pages = {104},
	keywords = {Astrophysics - Astrophysics of Galaxies, Galaxy: abundances, Galaxy: disk, Galaxy: evolution, Galaxy: formation, ISM: Abundances, stars: abundances},
	doi = {10.1088/0004-637X/807/1/104},
	author = {Ting, Yuan-Sen and Conroy, Charlie and Goodman, Alyssa}
}
@article {2015ApJ...815...23Z,
	title = {The Skeleton of the Milky Way},
	journal = {The Astrophysical Journal},
	volume = {815},
	year = {2015},
	month = {Dec},
	pages = {23},
	keywords = {Astrophysics - Astrophysics of Galaxies, Galaxy: kinematics and dynamics, Galaxy: structure, ISM: clouds},
	doi = {10.1088/0004-637X/815/1/23},
	author = {Zucker, Catherine and Battersby, Cara and Goodman, Alyssa}
}
@article {2014ApJ...797...53G,
	title = {The Bones of the Milky Way},
	journal = {The Astrophysical Journal},
	volume = {797},
	year = {2014},
	month = {Dec},
	pages = {53},
	keywords = {Astrophysics - Astrophysics of Galaxies, dust, extinction, galaxies: star formation, Galaxy: kinematics and dynamics, Galaxy: structure, ISM: clouds, ISM: Kinematics and Dynamics, ISM: structure},
	doi = {10.1088/0004-637X/797/1/53},
	author = {Goodman, Alyssa A. and Alves, Jo{\~a}o and Beaumont, Christopher N. and Benjamin, Robert A. and Michelle A. Borkin and Burkert, Andreas and Dame, Thomas M. and Jackson, James and Kauffmann, Jens and Robitaille, Thomas and Smith, Rowan J.}
}
@article {2014PLoSO...9j4798P,
	title = {How Do Astronomers Share Data? Reliability and Persistence of Datasets Linked in AAS Publications and a Qualitative Study of Data Practices among US Astronomers},
	journal = {PLoS ONE},
	volume = {9},
	year = {2014},
	month = {Aug},
	pages = {104798},
	doi = {10.1371/journal.pone.0104798},
	author = {Pepe, Alberto and Goodman, Alyssa and Muench, August and Merce Crosas and Erdmann, Christopher}
}
@conference {2014prpl.conf..101L,
	title = {The Link Between Magnetic Fields and Cloud/Star Formation},
	booktitle = {Protostars and Planets VI},
	year = {2014},
	pages = {101},
	keywords = {Astrophysics - Astrophysics of Galaxies},
	doi = {10.2458/azu_uapress_9780816531240-ch005},
	author = {Li, H. -B. and Goodman, A. and Sridharan, T.~K. and Houde, M. and Li, Z.-Y. and Novak, G. and Tang, K.~S.},
	editor = {Beuther, Henrik and Klessen, Ralf S. and Dullemond, Cornelis P. and Henning, Thomas}
}
@article {2014ApJS..214....3B,
	title = {The Milky Way Project: Leveraging Citizen Science and Machine Learning to Detect Interstellar Bubbles},
	journal = {The Astrophysical Journal Supplement Series},
	volume = {214},
	year = {2014},
	month = {Sep},
	pages = {3},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics, H II regions, ISM: bubbles, methods: data analysis, stars: formation},
	doi = {10.1088/0067-0049/214/1/3},
	author = {Beaumont, Christopher N. and Goodman, Alyssa A. and Kendrew, Sarah and Williams, Jonathan P. and Simpson, Robert}
}
@article {2014JSEdT..23..431S,
	title = {A New Approach to Developing Interactive Software Modules Through Graduate Education},
	journal = {Journal of Science Education and Technology},
	volume = {23},
	year = {2014},
	month = {Jun},
	pages = {431-440},
	keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Demonstrations, Physics - Physics Education, Science education, Simulations, Software development, Web tools, Web-based learning},
	doi = {10.1007/s10956-013-9474-4},
	author = {Sanders, Nathan E. and Faesi, Chris and Goodman, Alyssa A.}
}
@article {2014A\&A...567L...4P,
	title = {Smooth X-ray variability from \ensuremath\rho Ophiuchi A+B. A strongly magnetized primary B2 star?},
	journal = {Astronomy \& Astrophysics},
	volume = {567},
	year = {2014},
	month = {Jul},
	pages = {L4},
	keywords = {Astrophysics - Solar and Stellar Astrophysics, stars: activity, stars: early-type, stars: individual:\ensuremath\rhoOphiuchi, stars: magnetic field, starspots},
	doi = {10.1051/0004-6361/201424243},
	author = {Pillitteri, Ignazio and Wolk, Scott J. and Goodman, Alyssa and Sciortino, Salvatore}
}
@article {2014PLSCB..10E3542G,
	title = {Ten Simple Rules for the Care and Feeding of Scientific Data},
	journal = {PLoS Computational Biology},
	volume = {10},
	year = {2014},
	pages = {e1003542},
	keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Computer Science - Computers and Society, Computer Science - Digital Libraries},
	doi = {10.1371/journal.pcbi.1003542},
	author = {Goodman, Alyssa and Pepe, Alberto and Blocker, Alexander W. and Borgman, Christine L. and Cranmer, Kyle and Merce Crosas and Di Stefano, Rosanne and Gil, Yolanda and Groth, Paul and Hedstrom, Margaret and Hogg, David W. and Kashyap, Vinay and Mahabal, Ashish and Siemiginowska, Aneta and Slavkovic, Aleksandra}
}
@article {2013MNRAS.428.1606F,
	title = {Evidence for grain growth in molecular clouds: A Bayesian examination of the extinction law in Perseus},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {428},
	year = {2013},
	month = {Jan},
	pages = {1606-1622},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, dust, extinction, ISM: clouds, Methods: Statistical},
	doi = {10.1093/mnras/sts144},
	author = {Foster, Jonathan B. and Mandel, Kaisey S. and Pineda, Jaime E. and Covey, Kevin R. and Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {2013ApJ...770..141B,
	title = {Hierarchical Structure of Magnetohydrodynamic Turbulence in Position-position-velocity Space},
	journal = {The Astrophysical Journal},
	volume = {770},
	year = {2013},
	month = {Jun},
	pages = {141},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: structure, magnetohydrodynamics: MHD, turbulence},
	doi = {10.1088/0004-637X/770/2/141},
	author = {Burkhart, Blakesley and Lazarian, A. and Goodman, Alyssa and Rosolowsky, Erik}
}
@article {2013ApJ...777..173B,
	title = {Quantifying Observational Projection Effects Using Molecular Cloud Simulations},
	journal = {The Astrophysical Journal},
	volume = {777},
	year = {2013},
	month = {Nov},
	pages = {173},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, radiative transfer, techniques: image processing, techniques: spectroscopic},
	doi = {10.1088/0004-637X/777/2/173},
	author = {Beaumont, Christopher N. and Offner, Stella S.~R. and Shetty, Rahul and Glover, Simon C.~O. and Goodman, Alyssa A.}
}
@article {2012ApJ...752...55K,
	title = {Dust Spectral Energy Distributions in the Era of Herschel and Planck: A Hierarchical Bayesian-fitting Technique},
	journal = {The Astrophysical Journal},
	volume = {752},
	year = {2012},
	month = {Jun},
	pages = {55},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics, infrared: ISM, ISM: structure, methods: data analysis, Methods: Statistical, stars: formation},
	doi = {10.1088/0004-637X/752/1/55},
	author = {Kelly, Brandon C. and Shetty, Rahul and Stutz, Amelia M. and Kauffmann, Jens and Goodman, Alyssa A. and Launhardt, Ralf}
}
@article {2012MNRAS.420L..53O,
	title = {Observing turbulent fragmentation in simulations: predictions for CARMA and ALMA},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {420},
	year = {2012},
	month = {Feb},
	pages = {L53-L57},
	keywords = {Astrophysics - Solar and Stellar Astrophysics, stars: protostars, stars: starless cores},
	doi = {10.1111/j.1745-3933.2011.01194.x},
	author = {Offner, Stella S.~R. and Capodilupo, John and Schnee, Scott and Goodman, Alyssa A.}
}
@article {2012AN....333..505G,
	title = {Principles of high-dimensional data visualization in astronomy},
	journal = {Astronomische Nachrichten},
	volume = {333},
	year = {2012},
	month = {Jun},
	pages = {505},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics, cosmology: large-scale structure, ISM: clouds, methods: data analysis, Physics - Computational Physics, techniques: image processing, techniques: radial velocities},
	doi = {10.1002/asna.201211705},
	author = {Goodman, A.~A.}
}
@article {2012MNRAS.423.2579B,
	title = {A simple perspective on the mass-area relationship in molecular clouds},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {423},
	year = {2012},
	month = {Jul},
	pages = {2579-2586},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: structure, stars: formation},
	doi = {10.1111/j.1365-2966.2012.21061.x},
	author = {Beaumont, Christopher N. and Goodman, Alyssa A. and Alves, Jo{\~a}o. F. and Lombardi, Marco and Rom{\'a}n-Z{\'u}{\~n}iga, Carlos G. and Kauffmann, Jens and Lada, Charles J.}
}
@article {2011ApJ...742..105A,
	title = {A Bubbling Nearby Molecular Cloud: COMPLETE Shells in Perseus},
	journal = {The Astrophysical Journal},
	volume = {742},
	year = {2011},
	month = {Dec},
	pages = {105},
	keywords = {Astrophysics - Solar and Stellar Astrophysics, ISM: bubbles, ISM: individual objects: Perseus, outflows, stars: formation, stars: pre-main sequence, stars: winds, turbulence},
	doi = {10.1088/0004-637X/742/2/105},
	author = {Arce, H{\'e}ctor G. and Michelle A. Borkin and Goodman, Alyssa A. and Pineda, Jaime E. and Beaumont, Christopher N.}
}
@article {2011ApJ...741...14B,
	title = {Classifying Structures in the Interstellar Medium with Support Vector Machines: The G16.05-0.57 Supernova Remnant},
	journal = {The Astrophysical Journal},
	volume = {741},
	year = {2011},
	month = {Nov},
	pages = {14},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics, ISM: individual objects: G16.05-0.57 M17, ISM: supernova remnants, techniques: image processing},
	doi = {10.1088/0004-637X/741/1/14},
	author = {Beaumont, Christopher N. and Williams, Jonathan P. and Goodman, Alyssa A.}
}
@article {2011ApJ...743..201P,
	title = {The Enigmatic Core L1451-mm: A First Hydrostatic Core? Or a Hidden VeLLO?},
	journal = {The Astrophysical Journal},
	volume = {743},
	year = {2011},
	month = {Dec},
	pages = {201},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: individual objects: L1451 Perseus, ISM: molecules, stars: formation, stars: low-mass},
	doi = {10.1088/0004-637X/743/2/201},
	author = {Pineda, Jaime E. and Arce, H{\'e}ctor G. and Schnee, Scott and Goodman, Alyssa A. and Bourke, Tyler and Foster, Jonathan B. and Robitaille, Thomas and Tanner, Joel and Kauffmann, Jens and Tafalla, Mario and Caselli, Paola and Anglada, Guillem}
}
@article {2011ApJ...739L...2P,
	title = {Expanded Very Large Array Observations of the Barnard 5 Star-forming Core: Embedded Filaments Revealed},
	journal = {The Astrophysical Journal},
	volume = {739},
	year = {2011},
	month = {Sep},
	pages = {L2},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: individual objects: B5 Perseus Molecular Complex, ISM: molecules, stars: formation},
	doi = {10.1088/2041-8205/739/1/L2},
	author = {Pineda, Jaime E. and Goodman, Alyssa A. and Arce, H{\'e}ctor G. and Caselli, Paola and Longmore, Steven and Corder, Stuartt}
}
@conference {2011IAUS..270..511G,
	title = {A Guide to Comparisons of Star Formation Simulations with Observations},
	booktitle = {Computational Star Formation},
	series = {IAU Symposium},
	volume = {270},
	year = {2011},
	month = {Apr},
	pages = {511-519},
	keywords = {Astrophysics - Galaxy Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Simulations, star formation, statistical comparisons},
	doi = {10.1017/S1743921311000901},
	author = {Goodman, Alyssa A.},
	editor = {Alves, Jo{\~a}o. and Elmegreen, Bruce G. and Girart, Josep M. and Trimble, Virginia}
}
@article {2011ApJ...743...91O,
	title = {Radiation-hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons},
	journal = {The Astrophysical Journal},
	volume = {743},
	year = {2011},
	month = {Dec},
	pages = {91},
	keywords = {Astrophysics - Solar and Stellar Astrophysics, methods: numerical, molecular data, outflows, radiative transfer, stars: formation, stars: winds},
	doi = {10.1088/0004-637X/743/1/91},
	author = {Offner, Stella S.~R. and Lee, Eve J. and Goodman, Alyssa A. and Arce, H{\'e}ctor}
}
@article {2010ApJ...723..425D,
	title = {The Angular Momentum of Magnetized Molecular Cloud Cores: A Two-dimensional-Three-dimensional Comparison},
	journal = {The Astrophysical Journal},
	volume = {723},
	year = {2010},
	month = {Nov},
	pages = {425-439},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, ISM: clouds, ISM: Kinematics and Dynamics, ISM: magnetic fields, ISM: structure, radio lines: ISM, turbulence},
	doi = {10.1088/0004-637X/723/1/425},
	author = {Dib, Sami and Hennebelle, Patrick and Pineda, Jaime E. and Csengeri, Timea and Bontemps, Sylvain and Audit, Edouard and Goodman, Alyssa A.}
}
@article {2010ApJ...715.1170A,
	title = {The COMPLETE Survey of Outflows in Perseus},
	journal = {The Astrophysical Journal},
	volume = {715},
	year = {2010},
	month = {Jun},
	pages = {1170-1190},
	keywords = {Astrophysics - Solar and Stellar Astrophysics, ISM: clouds, ISM: individual objects: Perseus, ISM: Jets and Outflows, ISM: Kinematics and Dynamics, stars: formation, turbulence},
	doi = {10.1088/0004-637X/715/2/1170},
	author = {Arce, H{\'e}ctor G. and Michelle A. Borkin and Goodman, Alyssa A. and Pineda, Jaime E. and Halle, Michael W.}
}
@article {2010ApJ...712L.116P,
	title = {Direct Observation of a Sharp Transition to Coherence in Dense Cores},
	journal = {The Astrophysical Journal},
	volume = {712},
	year = {2010},
	month = {Mar},
	pages = {L116-L121},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: individual objects: B5 Perseus Molecular Complex, ISM: molecules, stars: formation},
	doi = {10.1088/2041-8205/712/1/L116},
	author = {Pineda, Jaime E. and Goodman, Alyssa A. and Arce, H{\'e}ctor G. and Caselli, Paola and Foster, Jonathan B. and Myers, Philip C. and Rosolowsky, Erik W.}
}
@article {2010ApJ...708..127S,
	title = {The Dust Emissivity Spectral Index in the Starless Core TMC-1C},
	journal = {The Astrophysical Journal},
	volume = {708},
	year = {2010},
	month = {Jan},
	pages = {127-136},
	keywords = {Astrophysics - Astrophysics of Galaxies, dust, extinction, stars: formation},
	doi = {10.1088/0004-637X/708/1/127},
	author = {Schnee, Scott and Enoch, Melissa and Noriega-Crespo, Alberto and Sayers, Jack and Terebey, Susan and Caselli, Paola and Foster, Jonathan and Goodman, Alyssa and Kauffmann, Jens and Padgett, Deborah and Rebull, Luisa and Sargent, Anneila and Shetty, Rahul}
}
@article {2010ApJ...723..457K,
	title = {The Dynamics of Dense Cores in the Perseus Molecular Cloud. II. The Relationship Between Dense Cores and the Cloud},
	journal = {The Astrophysical Journal},
	volume = {723},
	year = {2010},
	month = {Nov},
	pages = {457-475},
	keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics, ISM: clouds, ISM: individual objects: Perseus Molecular Cloud, ISM: Kinematics and Dynamics, ISM: molecules, turbulence},
	doi = {10.1088/0004-637X/723/1/457},
	author = {Kirk, Helen and Pineda, Jaime E. and Johnstone, Doug and Goodman, Alyssa}
}
@article {2010ApJ...712.1049S,
	title = {The Effect of Projection on Derived Mass-Size and Linewidth-Size Relationships},
	journal = {The Astrophysical Journal},
	volume = {712},
	year = {2010},
	month = {Apr},
	pages = {1049-1056},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: structure, METHODS: ANALYTICAL, stars: formation},
	doi = {10.1088/0004-637X/712/2/1049},
	author = {Shetty, Rahul and Collins, David C. and Kauffmann, Jens and Goodman, Alyssa A. and Rosolowsky, Erik W. and Norman, Michael L.}
}
@article {2010ApJ...712.1137K,
	title = {The Mass-Size Relation from Clouds to Cores. I. A New Probe of Structure in Molecular Clouds},
	journal = {The Astrophysical Journal},
	volume = {712},
	year = {2010},
	month = {Apr},
	pages = {1137-1146},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, methods: data analysis, stars: formation},
	doi = {10.1088/0004-637X/712/2/1137},
	author = {Kauffmann, J. and Pillai, T. and Shetty, R. and Myers, P.~C. and Goodman, A.~A.}
}
@article {2010ApJ...716..433K,
	title = {The Mass-size Relation from Clouds to Cores. II. Solar Neighborhood Clouds},
	journal = {The Astrophysical Journal},
	volume = {716},
	year = {2010},
	month = {Jun},
	pages = {433-445},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, methods: data analysis, stars: formation},
	doi = {10.1088/0004-637X/716/1/433},
	author = {Kauffmann, J. and Pillai, T. and Shetty, R. and Myers, P.~C. and Goodman, A.~A.}
}
@article {2010RMxAA..46..375L,
	title = {A reassessment of the kinematics of PV Cephei based on accurate proper motion measurements},
	journal = {Revista Mexicana de Astronom{\'\i}a y Astrof{\'\i}sica},
	volume = {46},
	year = {2010},
	pages = {375-383},
	keywords = {astrometry, Astrophysics - Galaxy Astrophysics, ISM: individual (PV Cep), ISM: Jets and Outflows, stars: pre-main sequence},
	author = {Loinard, L. and odr\'{\i}guez, L.~F. and G{\'o}mez, L. and ant{\'o}, J. and Raga, A.~C. and Goodman, A.~A. and Arce, H.~G.}
}
@article {2010ApJ...725.1327S,
	title = {Star Formation in the Taurus Filament L 1495: From Dense Cores to Stars},
	journal = {The Astrophysical Journal},
	volume = {725},
	year = {2010},
	month = {Dec},
	pages = {1327-1336},
	keywords = {Astrophysics - Astrophysics of Galaxies, dust, extinction, ISM: clouds, ISM: individual objects: L1495, ISM: structure, stars: formation},
	doi = {10.1088/0004-637X/725/1/1327},
	author = {Schmalzl, Markus and Kainulainen, Jouni and Quanz, Sascha P. and Alves, Jo{\~a}o and Goodman, Alyssa A. and Henning, Thomas and Launhardt, Ralf and Pineda, Jaime E. and Rom{\'a}n-Z{\'u}{\~n}iga, Carlos G.}
}
@article {2009ApJ...704..891L,
	title = {Anchoring Magnetic Field in Turbulent Molecular Clouds},
	journal = {The Astrophysical Journal},
	volume = {704},
	year = {2009},
	month = {Oct},
	pages = {891-897},
	keywords = {Astrophysics - Astrophysics of Galaxies, ISM: clouds, ISM: magnetic fields, polarization, stars: formation, turbulence},
	doi = {10.1088/0004-637X/704/2/891},
	author = {Li, Hua-bai and Dowell, C. Darren and Goodman, Alyssa and Hildebrand, Roger and Novak, Giles}
}
@article {2009ApJ...696..298F,
	title = {Dense Cores in Perseus: The Influence of Stellar Content and Cluster Environment},
	journal = {The Astrophysical Journal},
	volume = {696},
	year = {2009},
	month = {May},
	pages = {298-319},
	keywords = {Astrophysics - Galaxy Astrophysics, Astrophysics - Solar and Stellar Astrophysics, ISM: clouds, ISM: molecules, radio lines: ISM},
	doi = {10.1088/0004-637X/696/1/298},
	author = {Foster, Jonathan B. and Rosolowsky, Erik W. and Kauffmann, Jens and Pineda, Jaime E. and Michelle A. Borkin and Caselli, Paola and Myers, Phil C. and Goodman, Alyssa A.}
}
@article {2009ApJ...696.2234S,
	title = {The Effect of Line-of-Sight Temperature Variation and Noise on Dust Continuum Observations},
	journal = {The Astrophysical Journal},
	volume = {696},
	year = {2009},
	month = {May},
	pages = {2234-2251},
	keywords = {Astrophysics - Galaxy Astrophysics, Astrophysics - Solar and Stellar Astrophysics, dust, extinction, infrared: ISM, ISM: clouds, methods: miscellaneous, stars: formation},
	doi = {10.1088/0004-637X/696/2/2234},
	author = {Shetty, Rahul and Kauffmann, Jens and Schnee, Scott and Goodman, Alyssa A. and Ercolano, Barbara}
}
@article {2009ApJ...696..676S,
	title = {The Effect of Noise on the Dust Temperature-Spectral Index Correlation},
	journal = {The Astrophysical Journal},
	volume = {696},
	year = {2009},
	month = {May},
	pages = {676-680},
	keywords = {Astrophysics - Galaxy Astrophysics, Astrophysics - Solar and Stellar Astrophysics, dust, extinction, infrared: ISM, methods: miscellaneous},
	doi = {10.1088/0004-637X/696/1/676},
	author = {Shetty, Rahul and Kauffmann, Jens and Schnee, Scott and Goodman, Alyssa A.}
}
@article {2009ApJ...699L.134P,
	title = {The Perils of Clumpfind: The Mass Spectrum of Substructures in Molecular Clouds},
	journal = {The Astrophysical Journal},
	volume = {699},
	year = {2009},
	month = {Jul},
	pages = {L134-L138},
	keywords = {Astrophysics - Galaxy Astrophysics, ISM: clouds, ISM: individual: Perseus molecular complex, ISM: molecules, stars: formation},
	doi = {10.1088/0004-637X/699/2/L134},
	author = {Pineda, Jaime E. and Rosolowsky, Erik W. and Goodman, Alyssa A.}
}
@article {2009Natur.457...63G,
	title = {A role for self-gravity at multiple length scales in the process of star formation},
	journal = {Nature},
	volume = {457},
	year = {2009},
	month = {Jan},
	pages = {63-66},
	doi = {10.1038/nature07609},
	author = {Goodman, Alyssa A. and Rosolowsky, Erik W. and Michelle A. Borkin and Foster, Jonathan B. and Halle, Michael and Kauffmann, Jens and Pineda, Jaime E.}
}
@article {2009ApJ...692...91G,
	title = {The {\textquoteright}{\textquoteright}True{\textquoteright}{\textquoteright} Column Density Distribution in Star-Forming Molecular Clouds},
	journal = {The Astrophysical Journal},
	volume = {692},
	year = {2009},
	month = {Feb},
	pages = {91-103},
	keywords = {Astrophysics, dust, extinction, ISM: Abundances, ISM: individual: Perseus molecular complex, ISM: molecules},
	doi = {10.1088/0004-637X/692/1/91},
	author = {Goodman, Alyssa A. and Pineda, Jaime E. and Schnee, Scott L.}
}
@article {2008ApJS..175..509R,
	title = {An Ammonia Spectral Atlas of Dense Cores in Perseus},
	journal = {The Astrophysical Journal Supplement Series},
	volume = {175},
	year = {2008},
	month = {Apr},
	pages = {509-521},
	keywords = {Astrophysics, ISM: clouds, ISM: molecules, radio lines: ISM},
	doi = {10.1086/524299},
	author = {Rosolowsky, E.~W. and Pineda, J.~E. and Foster, J.~B. and Borkin, M.~A. and Kauffmann, J. and Caselli, P. and Myers, P.~C. and Goodman, A.~A.}
}
@article {2008ApJ...679..481P,
	title = {CO Isotopologues in the Perseus Molecular Cloud Complex: the X-factor and Regional Variations},
	journal = {The Astrophysical Journal},
	volume = {679},
	year = {2008},
	month = {May},
	pages = {481-496},
	keywords = {Astrophysics, dust, extinction, ISM: Abundances, ISM: individual: Perseus, ISM: molecules},
	doi = {10.1086/586883},
	author = {Pineda, Jaime E. and Caselli, Paola and Goodman, Alyssa A.}
}
@article {2008ApJ...684.1228S,
	title = {Dust Emission from the Perseus Molecular Cloud},
	journal = {The Astrophysical Journal},
	volume = {684},
	year = {2008},
	month = {Sep},
	pages = {1228-1239},
	keywords = {Astrophysics, dust, extinction, ISM: clouds, surveys},
	doi = {10.1086/590375},
	author = {Schnee, S. and Li, J. and Goodman, A.~A. and Sargent, A.~I.}
}
@article {2008ApJ...674..831F,
	title = {Hunting Galaxies to (and for) Extinction},
	journal = {The Astrophysical Journal},
	volume = {674},
	year = {2008},
	month = {Feb},
	pages = {831-845},
	keywords = {Astrophysics, dust, extinction, Galaxies: Fundamental Parameters, ISM: structure, stars: pre-main sequence},
	doi = {10.1086/524979},
	author = {Foster, Jonathan B. and Rom{\'a}n-Z{\'u}{\~n}iga, Carlos G. and Goodman, Alyssa A. and Lada, Elizabeth A. and Alves, Jo{\~a}o}
}
@article {2008ApJ...679.1338R,
	title = {Structural Analysis of Molecular Clouds: Dendrograms},
	journal = {The Astrophysical Journal},
	volume = {679},
	year = {2008},
	month = {Jun},
	pages = {1338-1351},
	keywords = {Astrophysics, ISM: clouds, ISM: structure, METHODS: ANALYTICAL, techniques: image processing},
	doi = {10.1086/587685},
	author = {Rosolowsky, E.~W. and Pineda, J.~E. and Kauffmann, J. and Goodman, A.~A.}
}
@article {2007ApJ...657..838S,
	title = {The Effect of Noise in Dust Emission Maps on the Derivation of Column Density, Temperature, and Emissivity Spectral Index},
	journal = {The Astrophysical Journal},
	volume = {657},
	year = {2007},
	month = {Mar},
	pages = {838-848},
	keywords = {Astrophysics, extinction, ISM: Dust, stars: formation, Submillimeter},
	doi = {10.1086/511054},
	author = {Schnee, S. and Kauffmann, J. and Goodman, A. and Bertoldi, F.}
}
@conference {2007prpl.conf..133G,
	title = {The Fragmentation of Cores and the Initial Binary Population},
	booktitle = {Protostars and Planets V},
	year = {2007},
	month = {Jan},
	pages = {133},
	keywords = {Astrophysics},
	author = {Goodwin, S.~P. and Kroupa, P. and Goodman, A. and Burkert, A.},
	editor = {Reipurth, Bo and Jewitt, David and Keil, Klaus}
}
@article {2007ApJ...671.1839S,
	title = {TMC-1C: An Accreting Starless Core},
	journal = {The Astrophysical Journal},
	volume = {671},
	year = {2007},
	month = {Dec},
	pages = {1839-1857},
	keywords = {Astrophysics, extinction, ISM: Dust, stars: formation, Submillimeter},
	doi = {10.1086/521577},
	author = {Schnee, S. and Caselli, P. and Goodman, A. and Arce, H.~G. and Ballesteros-Paredes, J. and Kuchibhotla, K.}
}
@article {2006ApJ...636L.105F,
	title = {Cloudshine: New Light on Dark Clouds},
	journal = {The Astrophysical Journal},
	volume = {636},
	year = {2006},
	month = {Jan},
	pages = {L105-L108},
	keywords = {Astrophysics, extinction, ISM: Dust, ISM: structure},
	doi = {10.1086/500131},
	author = {Foster, Jonathan B. and Goodman, Alyssa A.}
}
@article {2006ApJ...643..932R,
	title = {The COMPLETE Nature of the Warm Dust Shell in Perseus},
	journal = {The Astrophysical Journal},
	volume = {643},
	year = {2006},
	month = {Jun},
	pages = {932-944},
	keywords = {Astrophysics, extinction, infrared: ISM, ISM: Dust, ISM: H II Regions, ISM: individual (G159.6-18.5), radio lines: ISM},
	doi = {10.1086/502957},
	author = {Ridge, Naomi A. and Schnee, Scott L. and Goodman, Alyssa A. and Foster, Jonathan B.}
}
@article {2006AJ....131.2921R,
	title = {The COMPLETE Survey of Star-Forming Regions: Phase I Data},
	journal = {The Astronomical Journal},
	volume = {131},
	year = {2006},
	month = {Jun},
	pages = {2921-2933},
	keywords = {Astrophysics, ISM: clouds, stars: formation, surveys},
	doi = {10.1086/503704},
	author = {Ridge, Naomi A. and Di Francesco, James and Kirk, Helen and Li, Di and Goodman, Alyssa A. and Alves, Jo{\~a}o F. and Arce, H{\'e}ctor G. and Michelle A. Borkin and Caselli, Paola and Foster, Jonathan B. and Heyer, Mark H. and Johnstone, Doug and Kosslyn, David A. and Lombardi, Marco and Pineda, Jaime E. and Schnee, Scott L. and Tafalla, Mario}
}
@article {2006ApJ...640L..47S,
	title = {Estimating the Column Density in Molecular Clouds with Far-Infrared and Submillimeter Emission Maps},
	journal = {The Astrophysical Journal},
	volume = {640},
	year = {2006},
	month = {Mar},
	pages = {L47-L50},
	keywords = {Astrophysics, extinction, ISM: clouds, ISM: Dust, surveys},
	doi = {10.1086/503292},
	author = {Schnee, S. and Bethell, T. and Goodman, A.}
}
@article {2005ApJ...634..442S,
	title = {A COMPLETE Look at the Use of IRAS Emission Maps to Estimate Extinction and Dust Temperature},
	journal = {The Astrophysical Journal},
	volume = {634},
	year = {2005},
	month = {Nov},
	pages = {442-450},
	keywords = {Astrophysics, extinction, ISM: clouds, ISM: Dust, surveys},
	doi = {10.1086/491729},
	author = {Schnee, Scott L. and Ridge, Naomi A. and Goodman, Alyssa A. and Li, Jason G.}
}
@article {2005ApJ...624..254S,
	title = {Density and Temperature Structure of TMC-1C from 450 and 850 Micron Maps},
	journal = {The Astrophysical Journal},
	volume = {624},
	year = {2005},
	month = {May},
	pages = {254-266},
	keywords = {Astrophysics, extinction, ISM: Dust, stars: formation, Submillimeter},
	doi = {10.1086/429156},
	author = {Schnee, S. and Goodman, A.}
}
@article {2004ApJ...608..831G,
	title = {PV Cephei: Young Star Caught Speeding?},
	journal = {The Astrophysical Journal},
	volume = {608},
	year = {2004},
	month = {Jun},
	pages = {831-845},
	keywords = {Astrophysics, ISM: Herbig-Haro Objects, ISM: Individual: Alphanumeric: HH 315, ISM: Jets and Outflows, stars: formation, Stars: Individual: Constellation Name: PV Cephei, Stars: Kinematics},
	doi = {10.1086/383139},
	author = {Goodman, Alyssa A. and Arce, H{\'e}ctor G.}
}
@article {2003ApJ...588..881P,
	title = {The Spectral Correlation Function of Molecular Clouds: A Statistical Test for Theoretical Models},
	journal = {The Astrophysical Journal},
	volume = {588},
	year = {2003},
	month = {May},
	pages = {881-893},
	keywords = {Astrophysics, ISM: Individual: Name: Perseus, ISM: Individual: Name: Rosette Molecular Complex, ISM: Individual: Name: Taurus Molecular Cloud, ISM: Kinematics and Dynamics, radio lines: ISM, turbulence},
	doi = {10.1086/374240},
	author = {Padoan, Paolo and Goodman, Alyssa A. and Juvela, Mika}
}
@article {2002ApJ...575..928A,
	title = {Bow Shocks, Wiggling Jets, and Wide-Angle Winds: A High-Resolution Study of the Entrainment Mechanism of the PV Cephei Molecular (CO) Outflow},
	journal = {The Astrophysical Journal},
	volume = {575},
	year = {2002},
	month = {Aug},
	pages = {928-949},
	keywords = {Astrophysics, ISM: Herbig-Haro Objects, ISM: Individual: Alphanumeric: HH 315, ISM: Individual: Name: PV Cephei, ISM: Jets and Outflows, stars: formation},
	doi = {10.1086/341426},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {2002ApJ...575..911A,
	title = {The Great PV Cephei Outflow: A Case Study in Outflow-Cloud Interaction},
	journal = {The Astrophysical Journal},
	volume = {575},
	year = {2002},
	month = {Aug},
	pages = {911-927},
	keywords = {Astrophysics, ISM: clouds, ISM: Herbig-Haro Objects, ISM: Individual: Alphanumeric: HH 315, ISM: Individual: Name: PV Cephei, ISM: Jets and Outflows, stars: formation},
	doi = {10.1086/341427},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {2002ApJ...571..334B,
	title = {Velocity Structure of the Interstellar Medium as Seen by the Spectral Correlation Function},
	journal = {The Astrophysical Journal},
	volume = {571},
	year = {2002},
	month = {May},
	pages = {334-355},
	keywords = {Astrophysics, ISM: clouds, ISM: Kinematics and Dynamics, methods: data analysis, Methods: Statistical, turbulence},
	doi = {10.1086/339875},
	author = {Ballesteros-Paredes, Javier and V{\'a}zquez-Semadeni, Enrique and Goodman, Alyssa A.}
}
@article {2001ApJ...547..862P,
	title = {The Effects of Noise and Sampling on the Spectral Correlation Function},
	journal = {The Astrophysical Journal},
	volume = {547},
	year = {2001},
	month = {Feb},
	pages = {862-871},
	keywords = {Astrophysics, ISM: individual (Heiles{\textquoteright}s cloud 2), ISM: Kinematics and Dynamics, radio lines: ISM, turbulence},
	doi = {10.1086/318378},
	author = {Padoan, Paolo and Rosolowsky, Erik W. and Goodman, Alyssa A.}
}
@article {2001ApJ...554..132A,
	title = {The Episodic, Precessing Giant Molecular Outflow from IRAS 04239+2436 (HH 300)},
	journal = {The Astrophysical Journal},
	volume = {554},
	year = {2001},
	month = {Jun},
	pages = {132-151},
	keywords = {Astrophysics, HH 300), ISM: clouds, ISM: Herbig-Haro Objects, ISM: individual (B18, ISM: Jets and Outflows, stars: formation},
	doi = {10.1086/321334},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {2001ApJ...551L.171A,
	title = {The Mass-Velocity and Position-Velocity Relations in Episodic Outflows},
	journal = {The Astrophysical Journal},
	volume = {551},
	year = {2001},
	month = {Apr},
	pages = {L171-L174},
	keywords = {Astrophysics, ISM: Jets and Outflows, stars: formation, stars: mass loss},
	doi = {10.1086/320031},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {2001ApJ...555L..33P,
	title = {A New Method to Measure and Map the Gas Scale Height of Disk Galaxies},
	journal = {The Astrophysical Journal},
	volume = {555},
	year = {2001},
	month = {Jul},
	pages = {L33-L36},
	keywords = {Astrophysics, galaxies: ISM, Galaxies: Magellanic Clouds, Galaxies: Structure, turbulence},
	doi = {10.1086/321735},
	author = {Padoan, Paolo and Kim, Sungeun and Goodman, Alyssa and Staveley- Smith, Lister}
}
@article {2001ApJ...559.1005P,
	title = {Theoretical Models of Polarized Dust Emission from Protostellar Cores},
	journal = {The Astrophysical Journal},
	volume = {559},
	year = {2001},
	month = {Oct},
	pages = {1005-1018},
	keywords = {Astrophysics, ISM: clouds, ISM: Kinematics and Dynamics, polarization, radio continuum: ISM, Submillimeter, turbulence},
	doi = {10.1086/322504},
	author = {Padoan, Paolo and Goodman, Alyssa and Draine, B.~T. and Juvela, Mika and Nordlund, \rAke and R{\"o}gnvaldsson, {\"O}rn{\'o}lfur Einar}
}
@article {2001ApJ...553..227P,
	title = {The Turbulent Shock Origin of Proto-Stellar Cores},
	journal = {The Astrophysical Journal},
	volume = {553},
	year = {2001},
	month = {May},
	pages = {227-234},
	keywords = {Astrophysics, ISM: individual (Perseus, ISM: Kinematics and Dynamics, radio lines: ISM, Rosette, Taurus), turbulence},
	doi = {10.1086/320636},
	author = {Padoan, Paolo and Juvela, Mika and Goodman, Alyssa A. and Nordlund, \rAke}
}
@conference {2000prpl.conf..247W,
	title = {Polarized Light from Star-Forming Regions},
	booktitle = {Protostars and Planets IV},
	year = {2000},
	month = {May},
	pages = {247-272},
	author = {Weintraub, David A. and Goodman, Alyssa A. and Akeson, Rachel L.},
	editor = {Mannings, V. and Boss, A.~P. and Russell, S.~S.}
}
@article {1999AJ....117..707R,
	title = {BVRI Light Curves for 22 Type IA Supernovae},
	journal = {The Astronomical Journal},
	volume = {117},
	year = {1999},
	month = {Feb},
	pages = {707-724},
	keywords = {Astrophysics, Stars: Supernovae: General},
	doi = {10.1086/300738},
	author = {Riess, Adam G. and Kirshner, Robert P. and Schmidt, Brian P. and Jha, Saurabh and Challis, Peter and Garnavich, Peter M. and Esin, Ann A. and Carpenter, Chris and Grashius, Randy and Schild, Rudolph E. and Berlind, Perry L. and Huchra, John P. and Prosser, Charles F. and Falco, Emilio E. and Benson, Priscilla J. and Brice{\~n}o, C{\'e}sar and Brown, Warren R. and Caldwell, Nelson and dell{\textquoteright}Antonio, Ian P. and Filippenko, Alexei V. and Goodman, Alyssa A. and Grogin, Norman A. and Groner, Ted and Hughes, John P. and Green, Paul J. and Jansen, Rolf A. and Kleyna, Jan T. and Luu, Jane X. and Macri, Lucas M. and McLeod, Brian A. and McLeod, Kim K. and McNamara, Brian R. and McLean, Brian and Milone, Alejandra A.~E. and Mohr, Joseph J. and Moraru, Dan and Peng, Chien and Peters, Jim and Prestwich, Andrea H. and Stanek, Krzysztof Z. and Szentgyorgyi, Andy and Zhao, Ping}
}
@article {1999ApJ...517..264A,
	title = {An Extinction Study of the Taurus Dark Cloud Complex},
	journal = {The Astrophysical Journal},
	volume = {517},
	year = {1999},
	month = {May},
	pages = {264-281},
	keywords = {Astrophysics, extinction, INFRARED: ISM: CONTINUUM, ISM: Dust, ISM: INDIVIDUAL: NAME: TAURUS DARK CLOUD, techniques: photometric, techniques: spectroscopic},
	doi = {10.1086/307168},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {1999ApJ...512L.135A,
	title = {Measuring Galactic Extinction: A Test},
	journal = {The Astrophysical Journal},
	volume = {512},
	year = {1999},
	month = {Feb},
	pages = {L135-L138},
	keywords = {Astrophysics, extinction, INFRARED: ISM: CONTINUUM, ISM: Dust},
	doi = {10.1086/311885},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A.}
}
@article {1999ApJ...524..887R,
	title = {The Spectral Correlation Function: A New Tool for Analyzing Spectral Line Maps},
	journal = {The Astrophysical Journal},
	volume = {524},
	year = {1999},
	month = {Oct},
	pages = {887-894},
	keywords = {Astrophysics, ISM: structure, LINE: PROFILES, magnetohydrodynamics: MHD, Methods: Statistical, molecular data, turbulence},
	doi = {10.1086/307863},
	author = {Rosolowsky, Erik W. and Goodman, Alyssa A. and Wilner, David J. and Williams, Jonathan P.}
}
@article {1998ApJ...504..223G,
	title = {Coherence in Dense Cores. II. The Transition to Coherence},
	journal = {The Astrophysical Journal},
	volume = {504},
	year = {1998},
	month = {Sep},
	pages = {223-246},
	keywords = {ISM: clouds, ISM: Kinematics and Dynamics, ISM: structure, LINE: PROFILES},
	doi = {10.1086/306045},
	author = {Goodman, Alyssa A. and Barranco, Joseph A. and Wilner, David J. and Heyer, Mark H.}
}
@article {1998ApJ...504..207B,
	title = {Coherent Dense Cores. I. NH$_{3}$ Observations},
	journal = {The Astrophysical Journal},
	volume = {504},
	year = {1998},
	month = {Sep},
	pages = {207-222},
	keywords = {ISM: clouds, ISM: Kinematics and Dynamics, ISM: molecules, ISM: structure, turbulence},
	doi = {10.1086/306044},
	author = {Barranco, Joseph A. and Goodman, Alyssa A.}
}
@article {1998ApJ...499L..93A,
	title = {The Polarizing Power of the Interstellar Medium in Taurus},
	journal = {The Astrophysical Journal},
	volume = {499},
	year = {1998},
	month = {May},
	pages = {L93-L97},
	keywords = {Astrophysics, extinction, ISM: clouds, ISM: Dust, ISM: magnetic fields, polarization},
	doi = {10.1086/311337},
	author = {Arce, H{\'e}ctor G. and Goodman, Alyssa A. and Bastien, Pierre and Manset, Nadine and Sumner, Matthew}
}
@article {1998ApL\&C..37..109G,
	title = {Velocity Coherence in Dense Cores},
	journal = {Astrophysical Letters and Communications},
	volume = {37},
	year = {1998},
	month = {Jan},
	pages = {109},
	author = {Goodman, A.~A. and Barranco, J.~A. and Wilner, D.~J. and Heyer, M.~H.}
}
@article {1997ApJ...490..273L,
	title = {On the Efficiency of Grain Alignment in Dark Clouds},
	journal = {The Astrophysical Journal},
	volume = {490},
	year = {1997},
	month = {Nov},
	pages = {273-280},
	keywords = {Astrophysics, dust: extinction, ISM: clouds, polarization},
	doi = {10.1086/304874},
	author = {Lazarian, A. and Goodman, Alyssa A. and Myers, Philip C.}
}
@article {1997ApJ...482..334P,
	title = {Kinematics of the Ursa Major Molecular Clouds},
	journal = {The Astrophysical Journal},
	volume = {482},
	year = {1997},
	month = {Jun},
	pages = {334-354},
	keywords = {ISM: clouds, ISM: Individual: Name: Ursa Major, ISM: Kinematics and Dynamics, radio lines: ISM},
	doi = {10.1086/304136},
	author = {Pound, Marc W. and Goodman, Alyssa A.}
}
@article {1996ApJ...471..302T,
	title = {The Magnetic Fields in the Ophiuchus and Taurus Molecular Clouds},
	journal = {Astrophysical Journal},
	volume = {471},
	year = {1996},
	pages = {302},
	keywords = {ISM: clouds, ISM: INDIVIDUAL NAME: RHO OPHIUCHI CLOUD, ISM: INDIVIDUAL NAME: TAURUS MOLECULAR CLOUD, ISM: magnetic fields, ISM: molecules, polarization, stars: formation},
	doi = {10.1086/177970},
	author = {Troland, T.~H. and Crutcher, R.~M. and Goodman, A.~A. and Heiles, C. and Kazes, I. and Myers, P.~C.}
}
@article {1995ApJ...448..748G,
	title = {Does Near-Infrared Polarimetry Reveal the Magnetic Field in Cold Dark Clouds?},
	journal = {Astrophysical Journal},
	volume = {448},
	year = {1995},
	pages = {748},
	keywords = {extinction, INFRARED: ISM: CONTINUUM, ISM: clouds, ISM: Dust, ISM: INDIVIDUAL ALPHANUMERIC: L1755, ISM: magnetic fields, polarization},
	doi = {10.1086/176003},
	author = {Goodman, Alyssa A. and Jones, Terry J. and Lada, Elizabeth A. and Myers, Philip C.}
}
@inbook {1995LNP...459...82G,
	title = {Mapping Magnetic Fields in the ISM: Infrared and Sub-mm Polarimetry},
	booktitle = {The Physics and Chemistry of Interstellar Molecular Clouds, Proceedings of the 2nd Cologne-Zermatt Symposium, Held at Zermatt, Switzerland, 21 - 24 September 1993. Edited by G. Winnewisser and G. C. Pelz. Springer-Verlag Berlin Heidelberg New York. Also L},
	year = {1995},
	pages = {82},
	keywords = {Dark Clouds: Infrared Polarization, Dark Clouds: Magnetic Fields, Interstellar Matter: Infrared Polarization, Interstellar Matter: Magnetic Fields, Interstellar Matter: Sub-MM Radiation},
	doi = {10.1007/BFb0102096},
	author = {Goodman, A.~A.},
	editor = {Winnewisser, Gisbert and Pelz, Guido C.}
}
@article {1995ApJ...442..177M,
	title = {Observations of Magnetic Fields in Diffuse Clouds},
	journal = {Astrophysical Journal},
	volume = {442},
	year = {1995},
	pages = {177},
	keywords = {Astronomy, Flux Density, H I Regions, Interstellar Gas, Interstellar Magnetic Fields, ISM: clouds, ISM: magnetic fields, Line Of Sight, magnetic flux, Magnetohydrodynamic Waves, magnetohydrodynamics: MHD, Molecular Clouds, radio lines: ISM, Radio Observation, Radio Spectra, Spectrum Analysis, turbulence, Zeeman Effect},
	doi = {10.1086/175433},
	author = {Myers, P.~C. and Goodman, A.~A. and Gusten, R. and Heiles, C.}
}
@article {1995ApJ...455L.181G,
	title = {A Point in Favor of the Superparamagnetic Grain Hypothesis},
	journal = {Astrophysical Journal},
	volume = {455},
	year = {1995},
	pages = {L181},
	keywords = {extinction, ISM: Dust, ISM: magnetic fields, polarization},
	doi = {10.1086/309840},
	author = {Goodman, A.~A. and Whittet, D.~C.~B.}
}
@article {1994ApJ...433..117L,
	title = {Dense Cores in Dark Clouds. X. Ammonia Emission in the Perseus Molecular Cloud Complex},
	journal = {Astrophysical Journal},
	volume = {433},
	year = {1994},
	pages = {117},
	keywords = {Ammonia, Astronomical Spectroscopy, Astronomy, Emission Spectra, Interstellar Gas, ISM: INDIVIDUAL NAME: PERSEUS MOLECULAR CLOUD, ISM: molecules, Line Spectra, Molecular Clouds, Molecular Spectra, Radio Astronomy, radio lines: ISM, Radio Spectra, Sky Surveys (Astronomy), star formation, Stellar Mass},
	doi = {10.1086/174629},
	author = {Ladd, E.~F. and Myers, P.~C. and Goodman, A.~A.}
}
@article {1994ApJ...424..208G,
	title = {The Magnetic Field in the Ophiuchus Dark Cloud Complex},
	journal = {Astrophysical Journal},
	volume = {424},
	year = {1994},
	month = {Mar},
	pages = {208},
	keywords = {Astronomical Models, Astrophysics, Dark matter, ISM: magnetic fields, Line Of Sight, Line Spectra, magnetic fields, Molecular Clouds, Monatomic Gases, Ophiuchi Clouds, radio lines: ISM, Three Dimensional Models, Zeeman Effect},
	doi = {10.1086/173884},
	author = {Goodman, Alyssa A. and Heiles, Carl}
}
@article {1993ApJ...406..528G,
	title = {Dense Cores in Dark Clouds. VIII. Velocity Gradients},
	journal = {Astrophysical Journal},
	volume = {406},
	year = {1993},
	month = {Apr},
	pages = {528},
	keywords = {Angular Momentum, Angular Velocity, Astrophysics, Gradients, ISM: clouds, ISM: Kinematics and Dynamics, ISM: molecules, Molecular Clouds, star formation, stars: formation, Stellar Motions, Velocity Distribution},
	doi = {10.1086/172465},
	author = {Goodman, A.~A. and Benson, P.~J. and Fuller, G.~A. and Myers, P.~C.}
}
@article {1993ApJ...407..175C,
	title = {OH Zeeman Observations of Dark Clouds},
	journal = {Astrophysical Journal},
	volume = {407},
	year = {1993},
	pages = {175},
	keywords = {Astronomical Models, Astrophysics, Dark matter, Hydroxyl Radicals, Interstellar Magnetic Fields, ISM: clouds, ISM: magnetic fields, ISM: molecules, Spectral Line Width, Zeeman Effect},
	doi = {10.1086/172503},
	author = {Crutcher, R.~M. and Troland, T.~H. and Goodman, A.~A. and Heiles, C. and Kazes, I. and Myers, P.~C.}
}
@article {1992ApJ...399..108G,
	title = {The Structure of Magnetic Fields in Dark Clouds: Infrared Polarimetry in B216{\textendash}217},
	journal = {Astrophysical Journal},
	volume = {399},
	year = {1992},
	month = {Nov},
	pages = {108},
	keywords = {Astronomical Models, Astronomical Polarimetry, Astrophysics, Cosmic Dust, Dark matter, extinction, Infrared Astronomy, Interstellar Extinction, Interstellar Magnetic Fields, ISM: clouds, ISM: Dust, ISM: magnetic fields, Molecular Clouds, polarization, Taurus Constellation},
	doi = {10.1086/171907},
	author = {Goodman, Alyssa A. and Jones, Terry J. and Lada, Elizabeth A. and Myers, Philip C.}
}
@article {1991ApJ...376..561M,
	title = {Dense Cores in Dark Clouds. VI. Shapes},
	journal = {Astrophysical Journal},
	volume = {376},
	year = {1991},
	month = {Aug},
	pages = {561},
	keywords = {Astrophysics, Carbon Monoxide, Dark matter, Interstellar Matter, INTERSTELLAR: MOLECULES, Molecular Clouds, Nebulae, NEBULAE: STRUCTURE, star formation, stars: formation},
	doi = {10.1086/170305},
	author = {Myers, P.~C. and Fuller, G.~A. and Goodman, A.~A. and Benson, P.~J.}
}
@article {1991ApJ...373..509M,
	title = {On the Dispersion in Direction of Interstellar Polarization},
	journal = {Astrophysical Journal},
	volume = {373},
	year = {1991},
	pages = {509},
	keywords = {Astronomical Photometry, Astrophysics, CLUSTERS: OPEN, Dark matter, Dispersion, Interstellar Magnetic Fields, Interstellar Matter, INTERSTELLAR: MAGNETIC FIELDS, INTERSTELLAR: MATTER, Line Of Sight, Magnetohydrodynamics, Optical Polarization, polarization, Probability Distribution Functions, Star Clusters, Zeeman Effect},
	doi = {10.1086/170070},
	author = {Myers, P.~C. and Goodman, A.~A.}
}
@article {1990ApJ...359..363G,
	title = {Optical Polarization Maps of Star-forming Regions in Perseus, Taurus, and Ophiuchus},
	journal = {Astrophysical Journal},
	volume = {359},
	year = {1990},
	month = {Aug},
	pages = {363},
	keywords = {Astrophysics, Dark matter, Interstellar Magnetic Fields, INTERSTELLAR: MAGNETIC FIELDS, INTERSTELLAR: MATTER, Linear Polarization, Molecular Clouds, NEBULAE: GENERAL, Ophiuchi Clouds, Optical Polarization, Polarimetry, polarization, Sky Surveys (Astronomy), star formation},
	doi = {10.1086/169070},
	author = {Goodman, A.~A. and Bastien, P. and Myers, P.~C. and Menard, F.}
}
@article {1989JRASC..83..298B,
	title = {Linear polarization maps of three molecular clouds},
	journal = {Journal of the Royal Astronomical Society of Canada},
	volume = {83},
	year = {1989},
	pages = {298},
	keywords = {Molecular Clouds: Polarization, Star-Forming Regions: Polarization},
	author = {Bastien, P. and Goodman, A.~A. and Myers, P.~C. and M{\'e}nard, F.}
}
@article {1989ApJ...338L..61G,
	title = {Measurement of Magnetic Field Strength in the Dark Cloud Barnard 1},
	journal = {Astrophysical Journal},
	volume = {338},
	year = {1989},
	month = {Mar},
	pages = {L61},
	keywords = {Astrophysics, Dark matter, Hydroxyl Emission, Interstellar Magnetic Fields, Interstellar Matter, INTERSTELLAR: MATTER, Line Spectra, magnetic fields, magnetic flux, Molecular Clouds, star formation, Stellar Mass, Zeeman Effect},
	doi = {10.1086/185401},
	author = {Goodman, A.~A. and Crutcher, R.~M. and Heiles, C. and Myers, P.~C. and Troland, T.~H.}
}
@inbook {1989LNP...331..182G,
	title = {Measurement of the Magnetic Field in the Molecular Cloud B1},
	booktitle = {The Physics and Chemistry of Interstellar Molecular Clouds - MM and sub-mm observations in astrophysics, Proceedings of the Symposium, Zermatt, Switzerland, Sept. 22-25, 1988. Lecture Notes in Physics, Vol. 331, edited by G. Winnewisser and J. T. Armstron},
	year = {1989},
	pages = {182},
	keywords = {Astrophysics, Emission Spectra, Field Strength, Hydroxyl Emission, Interstellar Magnetic Fields, Line Of Sight, Line Spectra, Magnetic Measurement, Molecular Clouds, Zeeman Effect},
	doi = {10.1007/BFb0119475},
	author = {Goodman, A.~A. and Myers, P.~C. and Crutcher, R.~M. and Heiles, C. and Kaz{\`e}s, I. and Troland, T.~H.},
	editor = {Winnewisser, G. and Armstrong, J.~T.}
}
@article {1988ApJ...326L..27M,
	title = {Evidence for Magnetic and Virial Equilibrium in Molecular Clouds},
	journal = {Astrophysical Journal},
	volume = {326},
	year = {1988},
	month = {Mar},
	pages = {L27},
	keywords = {Astrophysics, Field Strength, H II regions, Interstellar Magnetic Fields, Interstellar Masers, Interstellar Matter, INTERSTELLAR: MAGNETIC FIELDS, INTERSTELLAR: MATTER, Molecular Clouds},
	doi = {10.1086/185116},
	author = {Myers, P.~C. and Goodman, A.~A.}
}
@inbook {1988LNP...315..128G,
	title = {Magnetic and Virial Equilibrium in Molecular Clouds},
	booktitle = {Molecular Clouds in the Milky Way and External Galaxies, Proceedings of the Conference held 2-4 November 1987 at University of Massachusetts, Amherst. Edited by R.L. Dickman, R.L. Snell, and J.S. Young. Lecture Notes in Physics, Vol. 315. Berlin: Springer},
	year = {1988},
	pages = {128},
	doi = {10.1007/3-540-50438-9_250},
	author = {Goodman, A.~A. and Myers, P.~C.},
	editor = {Dickman, Robert L. and Snell, Ronald L. and Young, Judith S.}
}
@article {1988ApJ...329..392M,
	title = {Magnetic Molecular Clouds: Indirect Evidence for Magnetic Support and Ambipolar Diffusion},
	journal = {Astrophysical Journal},
	volume = {329},
	year = {1988},
	month = {Jun},
	pages = {392},
	keywords = {Ambipolar Diffusion, Astrophysics, Centimeter Waves, Field Strength, Gravitational Fields, HYDROMAGNETICS, Interstellar Magnetic Fields, INTERSTELLAR: MAGNETIC FIELDS, INTERSTELLAR: MOLECULES, Magnetohydrodynamics, Molecular Clouds, Molecular Spectra, Virial Theorem, Zeeman Effect},
	doi = {10.1086/166385},
	author = {Myers, P.~C. and Goodman, A.~A.}
}
