Photometry of Fourteen Main Belt Asteroids
Abstract
The results of CCD photometry of 14 main belt asteroids obtained between 1996 and 2000 are presented. For most of them, the V or R composite lightcurves and the values of the synodic rotational period are derived. There exists no previous determination of the period for 11 of the observed objects.
- Publication:
-
Revista Mexicana de Astronomia y Astrofisica
- Pub Date:
- April 2003
- Bibcode:
- 2003RMxAA..39...69G
- Keywords:
-
- Minor planets;
- asteroids