Moving mesh simulations of star forming cores in magneto-gravo-turbulence
Star formation in our Galaxy occurs in molecular clouds that are self-gravitating, highly turbulent, and magnetized. We study the conditions under which cloud cores inherit large-scale magnetic field morphologies and how the field is governed by cloud turbulence. We present four moving-mesh simulati...
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| Hauptverfasser: | , , , , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
February 22, 2017
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| In: |
Arxiv
Year: 2017, Pages: 1-13 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1702.06133
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| Verfasserangaben: | Philip Mocz, Blakesley Burkhart, and Lars Hernquist, Harvard-Smithsonian Center for Astrophysics; Christopher F. McKee, Physics Department and Astronomy Department University of California at Berkeley; Volker Springel, Heidelberger Institut für Theoretische Studien and Zentrum für Astronomie der Universität Heidelberg, Astronomisches Recheninstitut |
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