Efficacy of early stellar feedback in low gas surface density environments

ABSTRACT. We present a suite of high-resolution radiation hydrodynamic simulations of a small patch (1 kpc2) of the interstellar medium (ISM) performed with ar

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Bibliographische Detailangaben
Hauptverfasser:	Kannan, Rahul (VerfasserIn) , Marinacci, Federico (VerfasserIn) , Simpson, Christine M. (VerfasserIn) , Glover, Simon (VerfasserIn) , Hernquist, Lars (VerfasserIn)
Dokumenttyp:	Article (Journal)
Sprache:	Englisch
Veröffentlicht:	2020
In:	Monthly notices of the Royal Astronomical Society Year: 2019, Jahrgang: 491, Heft: 2, Pages: 2088-2103
ISSN:	1365-2966
DOI:	10.1093/mnras/stz3078
Online-Zugang:	Verlag, Volltext: https://doi.org/10.1093/mnras/stz3078 Verlag: https://academic.oup.com/mnras/article/491/2/2088/5612205
Verfasserangaben:	Rahul Kannan, Federico Marinacci, Christine M. Simpson, Simon C.O. Glover and Lars Hernquist

Beschreibung
Zusammenfassung:	ABSTRACT. We present a suite of high-resolution radiation hydrodynamic simulations of a small patch (1 kpc2) of the interstellar medium (ISM) performed with ar
Beschreibung:	Advance access publication 2019 November 4 Gesehen am 21.02.2020
Beschreibung:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/stz3078