| Issue |
A&A
Volume 417, Number 2, April II 2004
|
|
|---|---|---|
| Page(s) | 499 - 514 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361:20034105 | |
| Published online | 19 March 2004 | |
Spectrophotometry of galaxies in the Virgo cluster *,**
II. The data
1
Università degli Studi di Milano - Bicocca, Piazza delle scienze 3, 20126 Milano, Italy
2
Laboratoire d'Astrophysique de Marseille, Traverse du Siphon, 13276 Marseille Cedex 12, France
Corresponding author: G. Gavazzi, giuseppe.gavazzi@mib.infn.it
Received:
23
July
2003
Accepted:
16
December
2003
Drift-scan mode (3600–6800 Å) spectra with 
resolution are presented
for 333 galaxies members of nearby clusters, covering the whole Hubble sequence. The majority (225) were obtained
for galaxies in the Virgo cluster where a completeness of 36%, if all Hubble types are considered, and of 51%,
restricting to late-types, was reached at 
16. Our data
can be therefore considered representative of the integrated spectral
properties of giant and dwarf galaxies in this cluster. Intensities and
equivalent widths (EWs) are derived for the principal lines, both in emission and
in absorption. Deblending of the underlying absorption from emission was achieved in most cases.
Key words: galaxies: clusters: individual: Virgo / techniques: spectroscopic / catalogs
Based on observations collected at the Observatoire de Haute Provence (OHP) (France), operated by the CNRS, at the European Southern Observatory (proposals 66.B-0026; 68.B-0505), at the Loiano telescope belonging to the University of Bologna (Italy) and at the Observatorio Astronomico National de San Pedro Martir (Mexico).
© ESO, 2004
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