Probing the initial conditions of high-mass star formation - II. Fragmentation, stability, and chemistry towards high-mass star-forming regions G29.96−0.02 and G35.20−1.74
A&A, 530 (2011) A118
Published online: 2011-05-23
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High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
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A Holistic Perspective on the Dynamics of G035.39-00.33: The Interplay between Gas and Magnetic Fields
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The TOP-SCOPE Survey of PGCCs: PMO and SCUBA-2 Observations of 64 PGCCs in the Second Galactic Quadrant
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Mapping the 13CO/C18O abundance ratio in the massive star-forming region G29.96−0.02
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Gravity drives the evolution of infrared dark hubs: JVLA observations of SDC13
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Searching for initial stage of massive star formation around the H II region G18.2–0.3
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Chuan-Peng Zhang and Guang-Xing LiMonthly Notices of the Royal Astronomical Society 469 (2) 2286 (2017)
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A Massive Prestellar Clump Hosting No High-mass Cores
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Are infrared dark clouds really quiescent?
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CN Zeeman and dust polarization in a high-mass cold clump
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CLOUD STRUCTURE OF GALACTIC OB CLUSTER-FORMING REGIONS FROM COMBINING GROUND- AND SPACE-BASED BOLOMETRIC OBSERVATIONS
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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. HoThe Astrophysical Journal 819 (2) 139 (2016)
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Investigating the structure and fragmentation of a highly filamentary IRDC
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FRAGMENTATION OF MOLECULAR CLUMPS AND FORMATION OF A PROTOCLUSTER
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MAGNETIC FIELDS IN HIGH-MASS INFRARED DARK CLOUDS
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Gas Dynamics and Magnetic Fields in Infrared Dark Clouds
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The Earliest Stages of Massive Clustered Star Formation: Fragmentation of Infrared Dark Clouds
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Gravity as main driver of non-thermal motions in massive star forming regions
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INITIAL FRAGMENTATION IN THE INFRARED DARK CLOUD G28.53−0.25
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THE ONSET OF MASSIVE STAR FORMATION: THE EVOLUTION OF TEMPERATURE AND DENSITY STRUCTURE IN AN INFRARED DARK CLOUD
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FRAGMENTATION OF MASSIVE DENSE CORES DOWN TO ≲ 1000 AU: RELATION BETWEEN FRAGMENTATION AND DENSITY STRUCTURE
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PROTOSTAR MASS FUNCTIONS IN YOUNG CLUSTERS
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