Issue |
EAS Publications Series
Volume 48, 2011
CRAL-2010 A Universe of Dwarf Galaxies
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Page(s) | 207 - 208 | |
Section | Dwarf Ellipticals | |
DOI | https://doi.org/10.1051/eas/1148046 | |
Published online | 11 July 2011 |
M. Koleva, Ph. Prugniel and I. Vauglin (eds)
EAS Publications Series, 48 (2011) 207–208
Faint Dwarf Galaxies in Nearby Clusters
1 Universitäts-Sternwarte München, Scheinerstr. 1, 81679 München, Germany
2 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany
3 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
Besides giant elliptical galaxies, a number of low-mass stellar systems inhabit the cores of galaxy clusters, such as dwarf elliptical galaxies (dEs/dSphs), ultra-compact dwarf galaxies (UCDs), and globular clusters. The detailed morphological examination of faint dwarf galaxies has, until recently, been limited to the Local Group (LG) and the two very nearby galaxy clusters Virgo and Fornax. Here, we compare the structural parameters of a large number of dEs/dSphs in the more distant clusters Hydra I and Centaurus to other dynamically hot stellar systems.
© EAS, EDP Sciences, 2011