Astron. Astrophys. Suppl. Ser. 137, 495-504
P. Severgnini1,4 - B. Garilli1 - P. Saracco2 - G. Chincarini2,3
Send offprint request: P. Severgnini
1 - IFCTR/CNR, Via Bassini, 15, 20133 Milano, Italy
e-mail: bianca@ifctr.mi.cnr.it
2 -
Osservatorio Astronomico di Brera-Merate, Milano, Italy
e-mail: saracco@merate.mi.astro.it
3 -
Dip. di Fisica, Univ. Milano, Via Celoria, 16, 20133 Milano, Italy
e-mail: guido@merate.mi.astro.it
4 -
Univ. degli Studi di Firenze, Dip. Astronomia e Scienza dello Spazio, Via Fermi 5,
50125 Firenze (Arcetri), Italy
e-mail: paolas@arcetri.astro.it
Received January 8; accepted April 21, 1999
We present H photometry for a sample of 95 galaxies in
Hickson Compact Groups obtained from observations of 31 groups.
The Catalogue lists isophotal and adaptive aperture (Kron aperture) flux measurements
for about 75
of the accordant galaxies inside the observed HCGs, 22 out of which
are upper limits. Non standard data reduction procedures have been used to obtain the
continuum subtracted H
images for each HCG of the target sample. Flux
calibration has also been performed in order to obtain H
luminosities for the
whole sample. Both the data reduction and calibration procedures are carefully
described in this paper. The new data listed in this Catalogue are of great importance
in understanding the star formation rate inside HCG galaxies and in giving new insights
on its dependence on galaxy interactions.
Key words: galaxies: clusters: general -- galaxies: evolution -- galaxies: interaction
Copyright The European Southern Observatory (ESO)