| Issue |
A&A
Volume 459, Number 2, November IV 2006
|
|
|---|---|---|
| Page(s) | 663 - 668 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361:20065877 | |
| Published online | 12 September 2006 | |
Photometry and models of selected main belt asteroids
III. 283 Emma, 665 Sabine, and 690 Wratislavia
1
Astronomical Observatory, Adam Mickiewicz University, Słoneczna 36, 60-286 Poznań, Poland e-mail: tmich@amu.edu.pl
2
Rolf Nevanlinna Institute, University of Helsinki PO Box 4, 00014 Helsinki, Finland
3
Research Institute of Astronomy, Kharkiv Karazin National University, Sums'ka 35, 61022 Kharkiv, Ukraine
Received:
22
June
2006
Accepted:
17
August
2006
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.
Key words: techniques: photometric / minor planets, asteroids
© ESO, 2006
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