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Testing the variability of the proton-to-electron mass ratio from observations of methanol in the dark cloud core L1498
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Very Large Array Ammonia Observations of the HH 111/HH 121 Protostellar System: A Detection of a New Source with a Peculiar Chemistry
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Properties of Dense Cores Embedded in Musca Derived from Extinction Maps and 13CO, C18O, and NH3 Emission Lines
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Astrochemical Properties of Planck Cold Clumps
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The Green Bank Ammonia Survey: First Results of NH3 Mapping of the Gould Belt
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UCLCHEM: A Gas-grain Chemical Code for Clouds, Cores, and C-Shocks*
WHAT IS CONTROLLING THE FRAGMENTATION IN THE INFRARED DARK CLOUD G14.225–0.506?: DIFFERENT LEVELS OF FRAGMENTATION IN TWIN HUBS
Gemma Busquet, Robert Estalella, Aina Palau, Hauyu Baobab Liu, Qizhou Zhang, Josep Miquel Girart, Itziar de Gregorio-Monsalvo, Thushara Pillai, Guillem Anglada and Paul T. P. Ho The Astrophysical Journal 819(2) 139 (2016) https://doi.org/10.3847/0004-637X/819/2/139
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Satoshi Ohashi, Ken'ichi Tatematsu, Patricio Sanhueza, et al. Monthly Notices of the Royal Astronomical Society 459(4) 4130 (2016) https://doi.org/10.1093/mnras/stw856
A rotating helical filament in the L1251 dark cloud
Ammonia excitation imaging of shocked gas towards the W28 gamma-ray source HESS J1801−233
Nigel I. Maxted, Phoebe de Wilt, Gavin P. Rowell, et al. Monthly Notices of the Royal Astronomical Society 462(1) 532 (2016) https://doi.org/10.1093/mnras/stw1687
INFALL/EXPANSION VELOCITIES IN THE LOW-MASS DENSE CORES L492, L694-2, AND L1521F: DEPENDENCE ON POSITION AND MOLECULAR TRACER
Jared Keown, Scott Schnee, Tyler L Bourke, James Di Francesco, Rachel Friesen, Paola Caselli, Philip Myers, Gerard Williger and Mario Tafalla The Astrophysical Journal 833(1) 97 (2016) https://doi.org/10.3847/1538-4357/833/1/97
MAGNETICALLY DOMINATED PARALLEL INTERSTELLAR FILAMENTS IN THE INFRARED DARK CLOUD G14.225-0.506*
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Revealing the dynamics of Class 0 protostellar discs with ALMA
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The role of non-ionizing radiation pressure in star formation: the stability of cores and filaments
How chemistry influences cloud structure, star formation, and the IMF
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MASSIVE QUIESCENT CORES IN ORION. VI. THE INTERNAL STRUCTURES AND A CANDIDATE OF TRANSITING CORE IN NGC 2024 FILAMENT
The RMS survey: ammonia mapping of the environment of massive young stellar objects
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PHYSICAL CONDITIONS OF THE EARLIEST PHASES OF MASSIVE STAR FORMATION: SINGLE-DISH AND INTERFEROMETRIC OBSERVATIONS OF AMMONIA AND CCS IN INFRARED DARK CLOUDS
MALT-45: a 7 mm survey of the southern Galaxy – I. Techniques and spectral line data
Christopher H. Jordan, Andrew J. Walsh, Vicki Lowe, et al. Monthly Notices of the Royal Astronomical Society 448(3) 2344 (2015) https://doi.org/10.1093/mnras/stv178
G305.136+0.068: A MASSIVE AND DENSE COLD CORE IN AN EARLY STAGE OF EVOLUTION
Properties of starless and prestellar cores in Taurus revealed by Herschel★ SPIRE/PACS imaging
K. A. Marsh, M. J. Griffin, P. Palmeirim, et al. Monthly Notices of the Royal Astronomical Society 439(4) 3683 (2014) https://doi.org/10.1093/mnras/stu219
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CORE AND FILAMENT FORMATION IN MAGNETIZED, SELF-GRAVITATING ISOTHERMAL LAYERS
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UNVEILING A NETWORK OF PARALLEL FILAMENTS IN THE INFRARED DARK CLOUD G14.225–0.506
Does a prestellar core always become Tracing? protostellar the evolution of cores from the prestellar to protostellar phase
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Properties of dense cores in clustered massive star-forming regions at high angular resolution
Álvaro Sánchez-Monge, Aina Palau, Francesco Fontani, et al. Monthly Notices of the Royal Astronomical Society 432(4) 3288 (2013) https://doi.org/10.1093/mnras/stt679
Chemical modeling of the L1498 and L1517B prestellar cores: CO and HCO+depletion