Volume 417, Number 2, April II 2004
|Page(s)||499 - 514|
|Published online||19 March 2004|
II. The data
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, firstname.lastname@example.org
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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