N-body/SPH study of dEs in a cluster environment
Until recently, dwarf elliptical galaxies (dEs) were mostly believed to be gas-less systems, having lost their interstellar medium (ISM) through a galactic wind or through ram pressure stripping in the dense cluster environment. However, recent H$\alpha$ and HI surveys indicate that some dEs in clus...
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Veröffentlicht in: | Proceedings of the International Astronomical Union 2005-03, Vol.1 (C198), p.372-373 |
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Sprache: | eng |
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