Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
ABSTRACT. Feedback from core collapse supernovae (SNe), the final stage of evolution of massive stars, is a key element in galaxy formation theory. The energy b
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
28 February 2022
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2022, Jahrgang: 512, Heft: 1, Pages: 199-215 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stac511 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stac511 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/512/1/199/6539346 |
| Verfasserangaben: | Benjamin W. Keller and J.M. Diederik Kruijssen |
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