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Modeling the kinematics and star formation history of Andromeda II by a gas-rich major merger of dwarf galaxies
Published online by Cambridge University Press: 21 March 2017
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.
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- Copyright © International Astronomical Union 2017