2004/01/01 by Giuseppe Gavazzi, Gavazzi, Giuseppe, Antonio Zaccardo +11 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Scientific Research and Discoveries #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20034105
published as Astron.Astrophys. 417 (2004) 499-514 · 17 Pages, 19 Figures, 9 Tables. Accepted for pubblication in A&A. Full tables and figures available at http://goldmine.mib.infn.it/papers/vccspec_2.html
arxiv created 2004/01/30 · openalex publication_date 2004/03/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
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.