Volume 384, Number 2, MarchIII 2002
|Page(s)||371 - 382|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 March 2002|
CRAL-Observatoire de Lyon, CNRS: UMR 142, 69561 St-Genis-Laval Cedex, France
Corresponding author: F. Simien, email@example.com
Accepted: 7 December 2001
We present the result of spectroscopic observations of a sample of 73 galaxies, completing the database published in this series of articles. The sample contains mostly low-luminosity early-type objects, including four dwarfs of the Local Group (in particular, deep spectra of NGC 205), 15 dEs or dS0s in the Virgo cluster, and UGC 05442, a spheroidal dwarf of the M 81 group. We have measured the central velocity dispersion for all but one object, and determined the major-axis rotation and velocity-dispersion profiles for 59 objects. For the current sample of diffuse (or dwarf) elliptical galaxies, we have compared stellar rotation to velocity dispersion; the analysis suggests that these objects may be nearly rotationally flattened, and therefore that anisotropy may be less important than previously thought.
Key words: galaxies: elliptical and lenticular, cD / galaxies: kinematics and dynamics / galaxies: fundamental parameters / galaxies: general
© ESO, 2002
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