Modeling the kinematics and star formation history of Andromeda II by a gas-rich major merger of dwarf galaxies
2016 ◽
Vol 11
(S321)
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pp. 132-132
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AbstractWe 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.
2002 ◽
Vol 388
(2)
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pp. 439-445
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2014 ◽
Vol 789
(2)
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pp. 96
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2018 ◽
Vol 14
(S344)
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pp. 429-436
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2013 ◽
Vol 778
(2)
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pp. 103
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