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Cited article:

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Filamentary Hierarchies and Superbubbles: Galactic Multiscale Magnetohydrodynamic Simulations of Giant Molecular Cloud to Star Cluster Formation

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Filament Accretion and Fragmentation in the Perseus Molecular Cloud

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On the evolution of the observed mass-to-length relationship for star-forming filaments

Jiancheng Feng, Rowan J Smith, Alvaro Hacar, Susan E Clark and Daniel Seifried
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Magnetic Fields and Fragmentation of Filaments in the Hub of California-X

Eun Jung Chung, Chang Won Lee, Woojin Kwon, Mario Tafalla, Shinyoung Kim, Archana Soam and Jungyeon Cho
The Astrophysical Journal 951 (1) 68 (2023)
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Molecular Clouds Associated with H ii Regions and Candidates within l = 106.°65 to 109.°50 and b = −1.°85 to 0.°95

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Merging filaments I: a race against collapse

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The isothermal evolution of a shock-filament interaction

K J A Goldsmith and J M Pittard
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L1495 revisited: a ppmap view of a star-forming filament

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Highly Embedded 8 μm cores of Star Formation in the Spiral Arms and Filaments of 15 Nearby Disk Galaxies

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Magnetized interstellar molecular clouds – II. The large-scale structure and dynamics of filamentary molecular clouds

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How do velocity structure functions trace gas dynamics in simulated molecular clouds?

R.-A. Chira, J. C. Ibáñez-Mejía, M.-M. Mac Low and Th. Henning
Astronomy & Astrophysics 630 A97 (2019)
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Star formation from dense shocked regions in supersonic isothermal magnetoturbulence

Philip Mocz and Blakesley Burkhart
Monthly Notices of the Royal Astronomical Society 480 (3) 3916 (2018)
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