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
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2018 May 17
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 478, Issue: 3, Pages: 4052-4067 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1297 |
| Online Access: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1297 Verlag, Volltext: https://academic.oup.com/mnras/article/478/3/4052/4998876 |
| Author Notes: | 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 |
| Summary: | 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 |
|---|---|
| Item Description: | Gesehen am 05.02.2019 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1297 |