Hot phase generation by supernovae in ISM simulations: resolution, chemistry, and thermal conduction

ABSTRACT Supernovae (SNe) generate hot gas in the interstellar medium (ISM), help setting the ISM structure, and support the driving of outflows. It is important to resolve the hot gas generation for galaxy formation simulations at solar mass and sub-parsec resolution that realize individual SN expl...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2020-06, Vol.495 (1), p.1035-1060
Hauptverfasser:	Steinwandel, Ulrich P, Moster, Benjamin P, Naab, Thorsten, Hu, Chia-Yu, Walch, Stefanie
Format:	Artikel
Sprache:	eng
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