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S Donkov, I Zh Stefanov, T V Veltchev and R S Klessen Monthly Notices of the Royal Astronomical Society 505(3) 3655 (2021) https://doi.org/10.1093/mnras/stab1572
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The parsec–scale relationship between ICO and AV in local molecular clouds
Cheoljong Lee, Adam K Leroy, Alberto D Bolatto, et al. Monthly Notices of the Royal Astronomical Society 474(4) 4672 (2018) https://doi.org/10.1093/mnras/stx2760
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FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN). III. Possible evidence for formation of NGC 6618 cluster in M 17 by cloud–cloud collision
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The dense cores and filamentary structure of the molecular cloud in Corona Australis: Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey
The Anatomy of the Column Density Probability Distribution Function (N-PDF)
Hope How-Huan Chen, Blakesley Burkhart, Alyssa Goodman and David C. Collins The Astrophysical Journal 859(2) 162 (2018) https://doi.org/10.3847/1538-4357/aabaf6
High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
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On the Appearance of Thresholds in the Dynamical Model of Star Formation
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Multitemperature mapping of dust structures throughout the Galactic Plane using the PPMAP tool with Herschel Hi-GAL data
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The driving of turbulence in simulations of molecular cloud formation and evolution
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An Estimation of the Star Formation Rate in the Perseus Complex
Statistical link between the structure of molecular clouds and their density distribution
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Herschelobservations of the Galactic H ii region RCW 79
A census of dense cores in the Taurus L1495 cloud from theHerschelGould Belt Survey
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Molecular clouds have power-law probability distribution functions
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