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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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 February 9
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 476, Heft: 2, Pages: 1796-1810 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty343 |
| Online-Zugang: | 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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| Verfasserangaben: | Shi Shao, Marius Cautun, Carlos S. Frenk, Robert J.J. Grand, Facundo A. Gómez, Federico Marinacci and Christine M. Simpson |
| Zusammenfassung: | 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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| Beschreibung: | Gesehen am 08.02.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty343 |