An uncertainty principle for star formation: II. A new method for characterizing the cloud-scale physics of star formation and feedback across cosmic history
ABSTRACT. The cloud-scale physics of star formation and feedback represent the main uncertainty in galaxy formation studies. Progress is hampered by the limite
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 May 2
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 479, Heft: 2, Pages: 1866-1952 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1128 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1128 Verlag, Volltext: https://academic.oup.com/mnras/article/479/2/1866/4990957 
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| Verfasserangaben: | J.M. Diederik Kruijssen, Andreas Schruba, Alexander P.S. Hygate, Chia-Yu Hu, Daniel T. Haydon and Steven N. Longmore |
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