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Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps

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We present an analysis of the relationship between the orientation of magnetic fields and filaments that form in 3D magnetohydrodynamic simulations of cluster-forming, turbulent molecular cloud clumps. We examine simulated cloud clumps with size scales of L ∼ 2-4 pc and densities of n ∼ 400-1000 cm−...

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Main Authors: Klassen, Mikhail (Author) , Pudritz, Ralph E. (Author) , Kirk, Helen (Author)
Format: Article (Journal)
Language:English
Published: 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 465, Issue: 2, Pages: 2254-2276
ISSN:1365-2966
DOI:10.1093/mnras/stw2889
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw2889
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Author Notes:Mikhail Klassen, Ralph E. Pudritz and Helen Kirk
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Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps by Klassen, Mikhail (Author) , Pudritz, Ralph E. (Author) , Kirk, Helen (Author) ,


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