Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries

0388364 - ASÚ 2013 RIV US eng J - Článek v odborném periodiku
Pravec, Petr - Scheirich, Peter - Vokrouhlický, D. - Harris, A. W. - Kušnirák, Peter - Hornoch, Kamil - Pray, D. P. - Higgins, D. - Galád, Adrián - Világi, J. - Gajdoš, Š. - Kornoš, L. - Oey, J. - Husárik, M. - Cooney, W.R. - Gross, J. - Terrell, D. - Durkee, R. - Pollock, J. - Reichart, D. E. - Ivarsen, K.M. - Haislip, J.B. - LaCluyze, A. - Krugly, Yu. N. - Gaftonyuk, N. M. - Stephens, R. - Dyvig, R. - Reddy, V. - Chiorny, V. G. - Vaduvescu, O. - Longa-Pena, P. - Tudorica, A. - Warner, B. D. - Masi, G. - Brinsfield, J. - Goncalves, R. - Brown, P. - Krzeminski, Z. - Gerashchenko, O. - Shevchenko, V. - Molotov, I.E. - Marchis, F.
Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries.
Icarus. Roč. 218, č. 1 (2012), s. 125-143. ISSN 0019-1035. E-ISSN 1090-2643
Grant CEP: GA ČR(CZ) GA205/05/0604; GA ČR GA205/09/1107
Institucionální podpora: RVO:67985815
Klíčová slova: asteroids * satellites of asteroids * photometry
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 3.161, rok: 2012

Parameters of 18 binary inner main-belt asteroids estimated/constrained. Orbit poles of small binary asteroids concentrate at high ecliptic latitudes.The YORP tilt of spins of binary parent bodies or primaries proposed as the cause.
Trvalý link: http://hdl.handle.net/11104/0217258