CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory

Details CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mpbu...35..161s&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Computer Science

Scientific paper

CCD photometry of three asteroids was obtained at the Universidad de Monterrey Observatory during 2007 April and 2008 March. These asteroids were observed on only one or two nights, but complete lightcurves were obtained due to relatively short rotation periods. The resulting synodic rotation periods and amplitudes are as follows: 811 Nauheima, 4.011 ± 0.006 h, 0.11 ± 0.03 mag; 3787 Aivazovskij, 2.97 ± 0.01 h, 0.18 ± 0.02 mag; and 5474 Gingasen, 3.628 ± 0.005 h, 0.16 ± 0.03 mag.

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