Photometry and models of selected main belt asteroids. III. 283 Emma, 665 Sabine, and 690 Wratislavia

Details Photometry and models of selected main belt asteroids. III. 283 Emma, 665 Sabine, and 690 Wratislavia Photometry and models of selected main belt asteroids. III. 283 Emma, 665 Sabine, and 690 Wratislavia

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...459..663m&link_type=abstract

Astronomy and Astrophysics, Volume 459, Issue 2, November IV 2006, pp.663-668

Astronomy and Astrophysics

Astrophysics

9

Techniques: Photometric, Minor Planets, Asteroids

Scientific paper

Photometric observations of 283 Emma (1998, 2000, 2001, 2004), 665 Sabine (1998, 1999, 2001, 2004, 2005), and 690 Wratislavia (1998, 2000, 2004, 2005-2006) carried out on 44 nights at two observatories are presented. Using all available lightcurves, the spin vectors, senses of rotation, and shape models for these three asteroids have been determined.

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