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
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| Main Authors: | , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
28 February 2022
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2022, Volume: 512, Issue: 1, Pages: 199-215 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stac511 |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stac511 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/512/1/199/6539346 
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| Author Notes: | Benjamin W. Keller and J.M. Diederik Kruijssen |
| Summary: | 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 |
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| Item Description: | Gesehen am 07.04.2022 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stac511 |