The multiplicity and anisotropy of galactic satellite accretion

Abstract. We study the incidence of group and filamentary dwarf galaxy accretion into Milky Way (MW) mass haloes using two types of hydrodynamical simulations:

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Bibliographic Details
Main Authors: Shao, Shi (Author) , Grand, Robert J. J. (Author)
Format: Article (Journal)
Language:English
Published: 2018 February 9
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 476, Issue: 2, Pages: 1796-1810
ISSN:1365-2966
DOI:10.1093/mnras/sty343
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty343
Verlag, Volltext: https://academic.oup.com/mnras/article/476/2/1796/4848305
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Author Notes:Shi Shao, Marius Cautun, Carlos S. Frenk, Robert J.J. Grand, Facundo A. Gómez, Federico Marinacci and Christine M. Simpson
Description
Summary:Abstract. We study the incidence of group and filamentary dwarf galaxy accretion into Milky Way (MW) mass haloes using two types of hydrodynamical simulations:
Item Description:Gesehen am 08.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty343