Volume 386, Number 1, April IV 2002
|Page(s)||134 - 139|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 April 2002|
Hα surface photometry of galaxies in the Virgo cluster III. Observations with INT and NOT 2.5 m telescopes *,**
Laboratoire d'Astronomie Spatiale, Traverse du Siphon, 13376 Marseille Cedex 12, France e-mail: Alessandro.Boselli@astrsp-mrs.fr,Jorge.Iglesias@astrsp-mrs.fr
2 Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, 18080, Granada, Spain e-mail: firstname.lastname@example.org
3 Università degli Studi di Milano-Bicocca, Piazza delle scienze 3, 20126 Milano, Italy
Corresponding author: A. Boselli, Giuseppe.Gavazzi@mib.infn.it
Accepted: 5 February 2002
We present Hα line imaging observations of 30 galaxies obtained at the 2.5 m INT and NOT telescopes. The observed galaxies are mostly BCD Virgo cluster galaxies. Hα+[NII] fluxes and equivalent widths, as well as images of all the detected targets are presented. With these observations, Hα data are available for 50% of the BCD galaxies listed in the VCC.
Key words: galaxies: photometry / galaxies: fundamental parameters
© ESO, 2002
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