0125005 - ASU-R 20020100 RIV US eng M - Část monografie knihy
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
Grant CEP: GA AV ČR IAA3003204; GA ČR GA205/99/0255
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: asteroids * structure * evolution processes
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

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.
Trvalý link: http://hdl.handle.net/11104/0023264