Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps
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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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2017
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2016, Jahrgang: 465, Heft: 2, Pages: 2254-2276 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw2889 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw2889
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| Verfasserangaben: | Mikhail Klassen, Ralph E. Pudritz and Helen Kirk |
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Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps
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