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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Hauptverfasser: Keller, Benjamin W. (VerfasserIn) , Kruijssen, Diederik (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 28 February 2022
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
Volltext
Verfasserangaben:Benjamin W. Keller and J.M. Diederik Kruijssen

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