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: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
23 August 2017
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| 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 
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| Verfasserangaben: | Jonas Frings, Andrea Macciò, Tobias Buck, Camilla Penzo, Aaron Dutton, Marvin Blank, Aura Obreja |
| Zusammenfassung: | 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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| Beschreibung: | Gesehen am 09.05.2018 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx2171 |