Volume 498, Number 1, April IV 2009
|Page(s)||313 - 320|
|Section||Planets and planetary systems|
|Published online||11 March 2009|
Photometry and models of selected main belt asteroids. VI. 160 Una, 747 Winchester, and 849 Ara*
Astronomical Observatory, Adam Mickiewicz University, Słoneczna 36, 60-286 Poznań, Poland e-mail: firstname.lastname@example.org
2 Geneva Observatory, 1290 Sauverny, Switzerland
3 Les Engarouines Observatory, 84570 Mallemort-du-Comtat, France
4 UNIQA Software Service, Gdańska 132, 90-520 Łódź, Poland
5 N. Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716 Warsaw, Poland
Accepted: 29 January 2009
We present a set of new photometric observations of three main belt asteroids: 160 Una, 747 Winchester, and 849 Ara. This, combined with the available data, allowed us to construct their physical models. The lightcurve inversion method was used to obtain their spins and shapes. We have resolved problems with the rotation period of 160 Una, and found it to be h, almost twice the value given in the literature.
Key words: techniques: photometric / minor planets, asteroids
© ESO, 2009
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