On the relevance of chaos for halo stars in the solar neighbourhood II
ABSTRACT. In a previous paper based on dark matter only simulations we show that, in the approximation of an analytic and static potential describing the stron
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 May 17
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 478, Heft: 3, Pages: 4052-4067 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1297 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1297 Verlag, Volltext: https://academic.oup.com/mnras/article/478/3/4052/4998876 
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| Verfasserangaben: | Nicolas P. Maffione, Facundo A. Gómez, Pablo M. Cincotta, Claudia M. Giordano, Robert J.J. Grand, Federico Marinacci, Rüdiger Pakmor, Christine M. Simpson, Volker Springel and Carlos S. Frenk |
| Zusammenfassung: | ABSTRACT. In a previous paper based on dark matter only simulations we show that, in the approximation of an analytic and static potential describing the stron |
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| Beschreibung: | Gesehen am 05.02.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1297 |