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• W3100598578 abstract "We have run high resolution N-body models simulating the encounter of a dwarf galaxy with a bright elliptical galaxy. The dwarf absorbs orbital angular momentum and shows counter-rotating features in the external regions of the galaxy. To explain the core-envelope kinematic decoupling observed in some dwarf galaxies in high-density environments requires nearly head-on collisions and very little dark matter bound to the dwarf. These kinematic structures appear under rather restrictive conditions. As a consequence, in a cluster like Virgo ~1% of dwarf galaxies may present counter-rotation formed by harassment." @default.
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• W3100598578 date "2005-12-01" @default.
• W3100598578 modified "2023-09-23" @default.
• W3100598578 title "Harassment origin for kinematic substructures in dwarf elliptical galaxies?" @default.
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• W3100598578 doi "https://doi.org/10.1051/0004-6361:20052670" @default.
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