Star formation and molecular hydrogen in dwarf galaxies: a non-equilibrium view

Abstract. We study the connection of star formation to atomic (H i) and molecular hydrogen (H2) in isolated, low-metallicity dwarf galaxies with high-resolutio

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Hauptverfasser: Hu, Chia-Yu (VerfasserIn) , Naab, Thorsten (VerfasserIn) , Walch, Stefanie (VerfasserIn) , Glover, Simon (VerfasserIn) , Clark, Paul C. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 07 March 2016
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Jahrgang: 458, Heft: 4, Pages: 3528-3553
ISSN:1365-2966
DOI:10.1093/mnras/stw544
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stw544
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/458/4/3528/2613831
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Verfasserangaben:Chia-Yu Hu, Thorsten Naab, Stefanie Walch, Simon C.O. Glover, Paul C. Clark

MARC

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