Photometry of Fourteen Main Belt Asteroids

Details Photometry of Fourteen Main Belt Asteroids Photometry of Fourteen Main Belt Asteroids

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxaa..39...69g&link_type=abstract

Revista Mexicana de Astronomía y Astrofísica Vol. 39, pp. 69-76 (2003) (http://www.astroscu.unam.mx/~rmaa/)

Astronomy and Astrophysics

Astronomy

Minor Planets, Asteroids

Scientific paper

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.

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