| Issue |
A&A
Volume 384, Number 2, MarchIII 2002
|
|
|---|---|---|
| Page(s) | 371 - 382 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361:20020071 | |
| Published online | 15 March 2002 | |
Kinematical data on early-type galaxies. VI. *,**
CRAL-Observatoire de Lyon, CNRS: UMR 142, 69561 St-Genis-Laval Cedex, France
Corresponding author: F. Simien, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
8
June
2001
Accepted:
7
December
2001
Abstract
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
Based on observations collected at the Observatoire de Haute-Provence.
Table 1 is also, and Tables 2 and 4 only, available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/384/371
© ESO, 2002
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