0125005 - ASU-R 20020100 RIV US eng M - Monography Chapter
Pravec, Petr - Harris, A. W. - Michalowski, T.
Asteroid rotations.
Asteroids III. Tucson: Univerzity of Arizona, 2002 - (Botthe, W.; Cellino, A.; Paolicchi, P.; Binzel, R.), s. 113-122
R&D Projects: GA AV ČR IAA3003204; GA ČR GA205/99/0255
Institutional research plan: CEZ:AV0Z1003909
Keywords : asteroids * structure * evolution processes
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

The rotations of asteroids larger than -40 km in diameter have a distribution close to Maxwellian that suggests that they are either original bodies of the asteroid main belt or its largest, collisionally evolved remnants.
Permanent Link: http://hdl.handle.net/11104/0023264