Abstract
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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CITATION STYLE
APA
Marciniak, A., Michałowski, T., Kaasalainen, M., Ďurech, J., Polińska, M., Kwiatkowski, T., … Roy, R. (2007). Photometry and models of selected main belt asteroids. Astronomy & Astrophysics, 473(2), 633–639. https://doi.org/10.1051/0004-6361:20077694
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