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Modeling the kinematics and star formation history of Andromeda II by a gas-rich major merger of dwarf galaxies
- Source :
- Proceedings of the International Astronomical Union. 11:132-132
- Publication Year :
- 2016
- Publisher :
- Cambridge University Press (CUP), 2016.
-
Abstract
- We present an evolutionary model for the origin of Andromeda II, a dwarf spheroidal satellite of M31. The model is an extension of the scenario proposed by Łokas et al. (2014) involving a major merger between two gas-rich disky dwarf galaxies.
Details
- ISSN :
- 17439221 and 17439213
- Volume :
- 11
- Database :
- OpenAIRE
- Journal :
- Proceedings of the International Astronomical Union
- Accession number :
- edsair.doi...........cea825506d035aa425d0097f51d6ad2d