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 from spiral-arm clouds. Here we determine the physical parameters of the central...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
2016
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1609.05911
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| Author Notes: | 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, A.J. Walsh |
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