Kraken reveals itself: the merger history of the Milky Way reconstructed with the E-MOSAICS simulations
Globular clusters (GCs) formed when the Milky Way experienced a phase of rapid assembly. We use the wealth of information contained in the Galactic GC population to quantify the properties of the satellite galaxies from which the Milky Way assembled.
Gespeichert in:
| Hauptverfasser: | , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2020 August 17
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2020, Jahrgang: 498, Heft: 2, Pages: 2472-2491 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/staa2452 |
| Online-Zugang: | Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa2452 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/498/2/2472/5893320 
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| Verfasserangaben: | J.M. Diederik Kruijssen, Joel L. Pfeffer, Mélanie Chevance, Ana Bonaca, Sebastian Trujillo-Gomez, Nate Bastian, Marta Reina-Campos, Robert A. Crain and Meghan E. Hughes |
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