Abstract
In 1984 we started an observational program on small asteroids (diameter lower than about 50 km) with the aim to enlarge the available dataset of the rotational periods of this size range objects. Here, we report the results obtained from photometric observations of ten small asteroids from August 1984 to January 1989 at the European Southern Observatory (La Silla, Chile). Reliable synodic rotational periods were determined for 8 asteroids.
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