Origin of chemically distinct discs in the Auriga cosmological simulations
The stellar disc of the Milky Way shows complex spatial and abundance structure that is central to understanding the key physical mechanisms responsible for shaping our Galaxy. In this study, we use six very high resolution cosmological zoom-in simulations of Milky Way-sized haloes to study the prev...
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 474, Heft: 3, Pages: 3629-3639 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx3025 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx3025 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/474/3/3629/4655198 
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| Verfasserangaben: | Robert J.J. Grand, Sebastián Bustamante, Facundo A. Gómez, Daisuke Kawata, Federico Marinacci, Rüdiger Pakmor, Hans-Walter Rix, Christine M. Simpson, Martin Sparre and Volker Springel |
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Origin of chemically distinct discs in the Auriga cosmological simulations
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