Photometry of Centaurs 1997 CU26 and 1999 UG5

Details Photometry of Centaurs 1997 CU26 and 1999 UG5 Photometry of Centaurs 1997 CU26 and 1999 UG5

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aard.conf..188p&link_type=abstract

ASTRONOMY AND ASTROPHYSICS Recent Developments. Proceedings of the 10th Portuguese Meeting. Held 27-28 July 2000 in CENTRA, Lisb

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present some preliminary results on BVRI photometry performed on two Centaurs at the 1.52 meter National Astronomical Observatory telescope at Calar Alto, Spain, during April 1999 and February 2000. From these observations, a search for periodic variations in the light curve of Centaur 1997 CU26 was made in both data sets. Also, the colour indices of Centaur 1999 UG5 were measured for the first time, indicating that this object is one of the reddest bodies in the Solar System.

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