Issue |
Astron. Astrophys. Suppl. Ser.
Volume 116, Number 3, May 1 1996
|
|
---|---|---|
Page(s) | 417 - 428 | |
DOI | https://doi.org/10.1051/aas:1996125 | |
Published online | 15 May 1996 |
Tidally-triggered disk thickening. I. Observations
1
Astronomical Institute of St. Petersburg State University, 198904 St. Petersburg, Russia
2
DEMIRM, Observatoire de Paris, 61 Av. de l'Observatoire, F-75014 Paris, France
Send offprint request to: F. Combes
Received:
18
July
1995
Accepted:
3
October
1995
As part of an investigation on what effect galaxy interactions have on the z-structure of the disks of involved galaxies, we present here new photometric data in the B, V, I passbands for a sample of 24 interacting systems and 7 non-interacting galaxies. Isophotes, total magnitudes and colours of all sample galaxies (67) are determined. Our estimates and the comparison with the published results show that the accuracy of our photometry is about 0.15 mag.
Key words: galaxies: interactions; photometry; spiral
© European Southern Observatory (ESO), 1996