Astron. Astrophys. Suppl. Ser.
Volume 121, Number 3, March 1997
|Page(s)||499 - 505|
|Published online||15 March 1997|
CCD photometry of the globular cluster Palomar 13*
Institute of Astronomy, Bulgarian Academy of Sciences, 72 Tsarigradsko chaussèe, BG – 1784 Sofia, Bulgaria
Send offprint request to: J. Borissova
Accepted: 21 May 1996
A new CCD photometry of the halo cluster Palomar 13 is used to construct a color - magnitude diagram in the Thuan-Gunn and the B, V photometric systems. The color-magnitude diagram of the cluster shows as already noted by Ortolani et al. (1985) an extremely poor red horizontal branch and a very sparsely populated giant branch. Seven BSS candidates are identified in the field of Palomar 13. The age of the cluster determined by fitting with the isochrones of Proffitt & Vanden Berg (1991) and Bergbusch & Vanden Berg (1992) and by a differential comparison of the color-magnitude diagram with that of Pal 5 is Gyr.
Key words: globular clusters: individual: Palomar 13 / Hertzprung / Russel diagram
© European Southern Observatory (ESO), 1997