Astron. Astrophys. Suppl. Ser.
Volume 125, Number 3, November I 1997
|Page(s)||459 - 469|
|Published online||15 November 1997|
Properties of nearby clusters of galaxies*
III. A 76, A 157, A 407, A 505, A 671, A 779, A 1700, A 2028, A 2040, A 2052, A 2063, A 2065, A 2593, A 2657, A 2670
Istituto Astronomico, Università di Roma "La Sapienza", via G. M. Lancisi 29, I-00161 Roma, Italy
2 Institute of Physics, Pedagogical University, Ul. Lesna 16, 25-509 Kielce, Poland
3 Department of Geophysics and Astronomy, University of British Columbia, 2219 Main Mall, Vancouver, BC, V6T 1Z4, Canada
Send offprint request to: D. Trèvese
Accepted: 29 January 1997
We present F band photometry, from digitized 48-inch Palomar plates, of 2818 galaxies brighter than m3+3 in 15 Abell clusters. For each galaxy, absolute coordinates, magnitude, size, ellipticity and orientation are given. For each cluster we provide finding charts and contour maps of the galaxy surface density. The absolute coordinates of the galaxies of other 8 clusters presented in the first paper of this series are also included.
Key words: galaxies: clusters of: general
Tables 3 to 17 of the present paper and Tables 18 to 25 (coordinates of the galaxies of Paper I) are available only in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1997