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
Hauptverfasser: Michielsen, Dolf, De Rijcke, S., Dejonghe, H.
Format: Artikel
Sprache:eng
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