The link between turbulence, magnetic fields, filaments, and star formation in the central molecular zone cloud G0.253+0.016
Star formation is primarily controlled by the interplay between gravity, turbulence, and magnetic fields. However, the turbulence and magnetic fields in molecular clouds near the Galactic center may differ substantially compared to spiral-arm clouds. Here we determine the physical parameters of the...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2016 November 28
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| In: |
The astrophysical journal
Year: 2016, Jahrgang: 832, Heft: 2, Pages: 154 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/0004-637X/832/2/143 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/0004-637X/832/2/143
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| Verfasserangaben: | C. Federrath, J.M. Rathborne, S.N. Longmore, J.M.D. Kruijssen, J. Bally, Y. Contreras, R.M. Crocker, G. Garay, J.M. Jackson, L. Testi, and A.J. Walsh |
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The link between turbulence, magnetic fields, filaments, and star formation in the central molecular zone cloud G0.253+0.016
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