Early Evolution of the Milky Way Satellite System
- Author(s)
- G. Hensler, M. Petrov
- Abstract
The dwarf spheroidal galaxies around the Milky Way (MW) belong to the
most poorly understood class of astronomical objects and serve as the
most challenging targets of astrophysical research for the reasons of
cosmology, evolution of satellite galaxies, faintest dwarf galaxies, and
accretion history of the MW. In order to yield a deeper insight into
these perspectives, numerical simulations from cosmological to galactic
scales and semi-analytical galaxy models have been undertaken by
numerous authors which are discussed here. Furthermore, a new
comprehensive chemo-dynamical approach is presented and its results are
highlighted.
- Organisation(s)
- Department of Astrophysics
- Volume
- 458
- Pages
- 367
- Publication date
- 08-2012
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/b68f1878-29b9-4ccc-8c1d-6945e4e83f4f