Are fibres in molecular cloud filaments real objects?

Abstract. We analyse the morphology and kinematics of dense filamentary structures produced in a numerical simulation of a star-forming cloud of 1.4 × 104 M⊙ e

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Hauptverfasser: Zamora-Avilés, Manuel (VerfasserIn) , Ballesteros-Paredes, Javier (VerfasserIn) , Hartmann, Lee (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2017 August 3
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 472, Heft: 1, Pages: 647-656
ISSN:1365-2966
DOI:10.1093/mnras/stx1995
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stx1995
Verlag, Volltext: https://academic.oup.com/mnras/article/472/1/647/4062210
Volltext
Verfasserangaben:Manuel Zamora-Avilés, Javier Ballesteros-Paredes and Lee W. Hartmann

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