Volume 416, Number 1, March II 2004
|Page(s)||353 - 366|
|Section||Planets and planetary systems|
|Published online||26 February 2004|
Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona
Astronomical Observatory, Adam Mickiewicz University, Słoneczna 36, 60-286 Poznań, Poland
2 Rolf Nevanlinna Institute, University of Helsinki PO Box 4, 00014 Helsinki, Finland
3 Copernicus Astronomical Center, Bartycka 18, 00-716 Warszawa, Poland
4 Research Institute of Astronomy, Kharkiv Karazin National University, Sums'ka 35, 61022 Kharkiv, Ukraine
5 Isaac Newton Institute of Chile, Crimean Branch
6 Institute of Space Sensor Technology and Planetary Exploration, Rutherford str. 2, 12489 Berlin, Germany
7 Institute of Astronomy, Rozhen National Observatory, PO Box 136, 4700 Smolyan, Bulgaria
8 Astroqueyras Association, Mairie, 05350 Saint Veran, France
9 Department of Experimental Physics & Astronomical Observatory, University of Szeged, 6720 Szeged, Dóm tér 9, Hungary
Corresponding author: T. Michałowski, email@example.com
Accepted: 24 November 2003
Photometric observations for 52 Europa (1995, 1997, 1999, 2000), 115 Thyra (1995, 1996, 1998, 2000), and 382 Dodona (1996, 1998, 1999, 2001) carried out at seven observatories are presented. Using all available lightcurves, the spin vectors, senses of rotation, and shape models of these three asteroids have been determined or refined.
Key words: techniques: photometric / minor planets, asteroids
© ESO, 2004
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