Dynamical friction for compound bodies

被引:11
作者
Dominguez-Tenreiro, R [1 ]
Gomez-Flechoso, MA [1 ]
机构
[1] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
关键词
methods; analytical; celestial mechanics; stellar dynamics;
D O I
10.1046/j.1365-8711.1998.01224.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the framework of the fluctuation-dissipation approach to dynamical friction, we derive an expression giving the orbital energy exchange experienced by a compound body, as it moves, interacting with a non-homogeneous discrete background. The body is assumed to be composed of particles endowed with a velocity spectrum and with a non-homogeneous spatial distribution. The Chandrasekhar formula is recovered in the limit of a point-like satellite with zero velocity dispersion and infinite temperature moving through a homogeneous infinite medium. In this same limit, but dropping the zero satellite velocity dispersion (sigma(s)) condition, the orbital energy loss is found to be smaller than in the sigma(s) = 0 case by a factor of up to an order of magnitude in some situations.
引用
收藏
页码:465 / 477
页数:13
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