Photometry and models of selected main belt asteroids. VI. 160 Una, 747 Winchester, and 849 Ara

Details Photometry and models of selected main belt asteroids. VI. 160 Una, 747 Winchester, and 849 Ara Photometry and models of selected main belt asteroids. VI. 160 Una, 747 Winchester, and 849 Ara

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...498..313m&link_type=abstract

Astronomy and Astrophysics, Volume 498, Issue 1, 2009, pp.313-320

Astronomy and Astrophysics

Astrophysics

5

Techniques: Photometric, Minor Planets, Asteroids

Scientific paper

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 11.033176 ± 0.000011 h, almost twice the value given in the literature.
Photometric data are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/498/313

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