Author: Carruba V. Machuca J. F. Gasparino H. P.
Publisher: Oxford University Press
ISSN: 0035-8711
Source: Monthly Notices of the Royal Astronomical Society, Vol.412, Iss.3, 2011-04, pp. : 2052-2062
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
Portrait of Theobalda as a young asteroid family
Monthly Notices of the Royal Astronomical Society, Vol. 407, Iss. 3, 2010-09 ,pp. :
Determination of Large Asteroid Masses by the Dynamical Method
Solar System Research, Vol. 38, Iss. 1, 2004-01 ,pp. :
Dynamical causes of asymmetry in the arrangement of gaps in the asteroid belt
By Markeev A.
Astronomy Letters, Vol. 27, Iss. 7, 2001-07 ,pp. :