The edge of galaxy formation: II. Evolution of Milky Way satellite analogues after infall

Abstract. In the first paper, we presented 27 hydrodynamical cosmological simulations of galaxies with total masses between 5 × 108 and 1010 M⊙. In this second

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Hauptverfasser: Frings, Jonas (VerfasserIn) , Buck, Tobias (VerfasserIn) , Penzo, Camilla (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 23 August 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 472, Heft: 3, Pages: 3378-3389
ISSN:1365-2966
DOI:10.1093/mnras/stx2171
Online-Zugang:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx2171
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/472/3/3378/4093087
Volltext
Verfasserangaben:Jonas Frings, Andrea Macciò, Tobias Buck, Camilla Penzo, Aaron Dutton, Marvin Blank, Aura Obreja

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