Astron. Astrophys. Suppl. Ser.
Volume 121, Number 3, March 1997
|Page(s)||507 - 551|
|Published online||15 March 1997|
MPI für Kernphysik, Postfach 103980, D–69117 Heidelberg, Germany
2 DEMIRM, Observatoire de Paris, 61 Av. de l'Observatoire, 75014 Paris, France
3 present address: Laboratoire d'Astronomie Spatiale, Traverse du Siphon, F-13376 Marseille Cedex 12, France
4 Università degli Studi di Milano, Via Celoria 16, 20133, Milano, Italy
5 Osservatorio Astronomico di Brera, Via Brera 28, 20121 Milano, Italy
6 MPI für Astronomie, Königstuhl, D–69117 Heidelberg, Germany
Send offprint request to: R.J. Tuffs
Accepted: 3 June 1996
Near Infrared ( band) surface photometry has been obtained for 102 (88 late-type) Virgo cluster galaxies. A subset of 20 galaxies was also imaged in the H band. Magnitudes and diameters within the 21.5 and 22.0 mag arcsec-2 isophote, concentration indices and total H and magnitudes are derived. Basic statistical properties of a complete sample of spiral galaxies spanning the range are given.
Key words: galaxies: fundamental parameters / galaxies: photometry / infrared: galaxies / galaxies: clusters: Virgo cluster
based on observations taken at the Calar Alto Observatory, operated by the Max-Planck-Institut für Astronomie (Heidelberg) jointly with the Spanish National Commission for Astronomy.
Tables 3, 5 and 6 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (18.104.22.168) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1997