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:
Bibliographic Details
Main Authors: Maffione, Nicolas P. (Author) , Grand, Robert J. J. (Author) , Springel, Volker (Author) , Pakmor, Rüdiger (Author)
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
Get full text
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
Description
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