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Cited article:

GRAVITATIONAL STABILITY OF A CYLINDRICAL PLASMA WITH AN AZIMUTHAL AND AN AXIAL MAGNETIC FIELD

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LINE PROFILES OF CORES WITHIN CLUSTERS. I. THE ANATOMY OF A FILAMENT

Rowan J. Smith, Rahul Shetty, Amelia M. Stutz and Ralf S. Klessen
The Astrophysical Journal 750 (1) 64 (2012)
https://doi.org/10.1088/0004-637X/750/1/64

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THE STAR FORMATION RATE OF TURBULENT MAGNETIZED CLOUDS: COMPARING THEORY, SIMULATIONS, AND OBSERVATIONS

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The Pipe Nebula as seen withHerschel: formation of filamentary structures by large-scale compression?

N. Peretto, Ph. André, V. Könyves, et al.
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Profiling filaments: comparing near-infrared extinction and submillimetre data in TMC-1

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Astronomy & Astrophysics 544 A50 (2012)
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The JCMT Nearby Galaxies Legacy Survey — VIII. CO data and the LCO(3-2)-LFIR correlation in the SINGS sample

C. D. Wilson, B. E. Warren, F. P. Israel, et al.
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THE IMPACT OF THERMODYNAMICS ON GRAVITATIONAL COLLAPSE: FILAMENT FORMATION AND MAGNETIC FIELD AMPLIFICATION

Thomas Peters, Dominik R. G. Schleicher, Ralf S. Klessen, et al.
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On the formation of very metal poor stars: the case of SDSS J1029151+172927

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FILAMENTARY STAR FORMATION: OBSERVING THE EVOLUTION TOWARD FLATTENED ENVELOPES

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The Astrophysical Journal 761 (2) 171 (2012)
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EXPANDED VERY LARGE ARRAY OBSERVATIONS OF THE BARNARD 5 STAR-FORMING CORE: EMBEDDED FILAMENTS REVEALED

Jaime E. Pineda, Alyssa A. Goodman, Héctor G. Arce, et al.
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Filaments and ridges in Vela C revealed byHerschel: from low-mass to high-mass star-forming sites

T. Hill, F. Motte, P. Didelon, et al.
Astronomy & Astrophysics 533 A94 (2011)
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