CCD sequences have been measured in 10 southern Abell clusters. Table 1 (click here)
gives the cluster coordinates according to Abell et al. (1989). The
final catalogue, given in Tables 2 to 20, contains
B, V and R magnitudes for 117 galaxies and 162 stars with 12.7 < V <
21.0. Column 2 gives the object type, S for star, G for galaxy.
The positions were measured from scans of the direct Schmidt plates with one
of the PDS 2020 
machines at the Astronomisches Institut,
Münster, Germany. Their accuracy is between 
and 
.
Acknowledgements
We thank Dr. R.S. Stobie for allocation of observing time at SAAO/Sutherland. We also thank the SAAO staff for assistance during the observations. It is a pleasure for GS to thank the Department of Mathematics, Applied Mathematics and Astronomy of the University of South Africa for the invitation, the financial support and for the hospitality during the stay at the University where a part of this publication was prepared. GS further thanks the Internationales Büro des Forschungszentrum Jülich and the BMBF for the financial support of the observing run under number S3539000. Special thanks go to Prof. W. Seitter and the other members of the Muenster Redshift Project (MRSP) for many useful discussions. Dr. A. Bruch kindly provided the programmes for magnitude transformation from the CCD system to the standard system. This work is part of the MRSP. Financial support of the MRSP by the DFG under numbers Se 345/14-1,2,3 and Se 345/21-1 is gratefully acknowledged. Finally BC, RD, GS and RU thank Walter F. Wargau for a very fruitful and sucessful collaboration during the last years. Walter died shortly after this paper has been submitted. We will miss him.