Star formation in a high-pressure environment: an SMA view of the Galactic centre dust ridge
The star formation rate in the Central Molecular Zone (CMZ) is an order of magnitude lower than predicted according to star formation relations that have been calibrated in the disc of our own and nearby galaxies. Understanding how and why star formation appears to be different in this region is cru...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 474, Heft: 2, Pages: 2373-2388 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx2898 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx2898 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/474/2/2373/4622962 
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| Verfasserangaben: | D.L. Walker, S.N. Longmore, Q. Zhang, C. Battersby, E. Keto, J.M.D. Kruijssen, A. Ginsburg, X. Lu, J.D. Henshaw, J. Kauffmann, T. Pillai, E.A.C. Mills, A.J. Walsh, J. Bally, L.C. Ho, K. Immer and K.G. Johnston |
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Star formation in a high-pressure environment: an SMA view of the Galactic centre dust ridge
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