Star formation rates and efficiencies in the Galactic Centre
The inner few hundred parsecs of the Milky Way harbours gas densities, pressures, velocity dispersions, an interstellar radiation field and a cosmic ray ionization rate orders of magnitude higher than the disc; akin to the environment found in star-forming galaxies at high redshift. Previous studies...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
21 April 2017
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 469, Heft: 2, Pages: 2263-2285 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx941 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx941
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| Verfasserangaben: | A.T. Barnes, S.N. Longmore, C. Battersby, J. Bally, J.M.D. Kruijssen, J.D. Henshaw, and D.L. Walker |
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Star formation rates and efficiencies in the Galactic Centre
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