The edge of galaxy formation: II. Evolution of Milky Way satellite analogues after infall

Abstract. In the first paper, we presented 27 hydrodynamical cosmological simulations of galaxies with total masses between 5 × 108 and 1010 M⊙. In this second

Saved in:

Bibliographic Details
Main Authors:	Frings, Jonas (Author) , Buck, Tobias (Author) , Penzo, Camilla (Author)
Format:	Article (Journal)
Language:	English
Published:	23 August 2017
In:	Monthly notices of the Royal Astronomical Society Year: 2017, Volume: 472, Issue: 3, Pages: 3378-3389
ISSN:	1365-2966
DOI:	10.1093/mnras/stx2171
Online Access:	Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx2171 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/472/3/3378/4093087
Author Notes:	Jonas Frings, Andrea Macciò, Tobias Buck, Camilla Penzo, Aaron Dutton, Marvin Blank, Aura Obreja

Description
Summary:	Abstract. In the first paper, we presented 27 hydrodynamical cosmological simulations of galaxies with total masses between 5 × 108 and 1010 M⊙. In this second
Item Description:	Gesehen am 09.05.2018
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/stx2171