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PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions

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The evolution of temperature and density structures of OB cluster-forming molecular clumps

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Systematic Investigation of Dust and Gaseous CO in 12 Nearby Molecular Clouds

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Network of Star Formation: Fragmentation Controlled by Scale-dependent Turbulent Pressure and Accretion onto the Massive Cores Revealed in the Cygnus-X GMC Complex

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Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies

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Molecular Clouds in the Second Quadrant of the Milky Way Midplane from l = 104.°75 to l = 119.°75 and b = −5.°25 to b = 5.°25

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Evolution of the Gas Density in a Simulated Star-forming Cloud with Stellar Feedback

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Density profile of a self-gravitating polytropic turbulent fluid in the context of ensembles of molecular clouds

S Donkov, I Zh Stefanov, T V Veltchev and R S Klessen
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ALMA–IRDC: dense gas mass distribution from cloud to core scales

A T Barnes, J D Henshaw, F Fontani, et al.
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On filament fragmentation and the impact of ambient environment on it

S V Anathpindika and J Di Francesco
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sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling

Karen Pardos Olsen, Blakesley Burkhart, Mordecai-Mark Mac Low, Robin G. Treß, Thomas R. Greve, David Vizgan, Jay Motka, Josh Borrow, Gergö Popping, Romeel Davé, Rowan J. Smith and Desika Narayanan
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SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation

Yutaka Hirai, Michiko S Fujii and Takayuki R Saitoh
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The Organization of Cloud-scale Gas Density Structure: High-resolution CO versus 3.6 μm Brightness Contrasts in Nearby Galaxies

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Three-dimensional Structure and Dust Extinction in the Small Magellanic Cloud

Petia Yanchulova Merica-Jones, Karin M. Sandstrom, L. Clifton Johnson, Andrew E. Dolphin, Julianne J. Dalcanton, Karl Gordon, Julia Roman-Duval, Daniel R. Weisz and Benjamin F. Williams
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Generalized Transport Equation for the Autocovariance Function of the Density Field and Mass Invariant in Star-forming Clouds

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The Cloud Factory II: gravoturbulent kinematics of resolved molecular clouds in a galactic potential

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Simulations of the star-forming molecular gas in an interacting M51-like galaxy

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The turbulence driving parameter of molecular clouds in disc galaxies

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A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces. II. The Bottleneck to Collapse Set by Cloud–Environment Decoupling

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Formation of the Musca filament: evidence for asymmetries in the accretion flow due to a cloud–cloud collision

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The column density structure of Orion A depicted by N-PDF

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https://doi.org/10.3847/1538-4357/ab77b5