## Abstract We present models of the formation and evolution of isolated dwarf galaxies. The models follow the evolution of an initially homogeneous gas cloud collapsing in a preβexisting darkβmatter halo. These simplified initial conditions are supported by the merger trees of isolated dwarf galax
Evolution of galaxies in pairs: Learning from simulations
β Scribed by P. Di Matteo; F. Combes; I. Chilingarian; A.-L. Melchior; B. Semelin
- Publisher
- John Wiley and Sons
- Year
- 2008
- Tongue
- English
- Weight
- 235 KB
- Volume
- 329
- Category
- Article
- ISSN
- 0004-6337
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