| Issue |
A&A
Volume 386, Number 1, April IV 2002
|
|
|---|---|---|
| Page(s) | 134 - 139 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361:20020216 | |
| Published online | 15 April 2002 | |
Hα surface photometry of galaxies in the Virgo cluster III. Observations with INT and NOT 2.5 m telescopes *,**
1
Laboratoire d'Astronomie Spatiale, Traverse du Siphon, 13376 Marseille Cedex 12, France e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
,This email address is being protected from spambots. You need JavaScript enabled to view it.
2
Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, 18080, Granada, Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
3
Università degli Studi di Milano-Bicocca, Piazza delle scienze 3, 20126 Milano, Italy
Corresponding author: A. Boselli, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
3
December
2001
Accepted:
5
February
2002
Abstract
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
Based on observations taken at the INT and NOT telescopes, operated on the island of La Palma by the ING and NOT teams in the Spanish Observatorio del Roque de Los Muchachos of the Instituto de Astrofísica de Canarias.
Figure 1 is only available in electronic form at http://www.edpsciences.org
© ESO, 2002
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