Formation of the planetary sequence in a highly flattened disk of frequently colliding planetesimals

被引：0

作者：

Griv, E ^{[1
]}

Gedalin, M ^{[1
]}

Eichler, D ^{[1
]}

Yuan, C ^{[1
]}

机构：

[1] Ben Gurion Univ Negev, Dept Phys, IL-84105 Beer Sheva, Israel

来源：

PLANETARY SYSTEMS IN THE UNIVERSE OBSERVATION, FORMATION AND EVOLUTION | 2004年 / 202期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The kinetic theory is used to study the evolution of the selfgravitating disk of planetesimals. The effects of frequent collisions between planetesimals are taken into account by using a Krook integral in the Boltzmann kinetic equation. It is shown that as a result of an aperiodic collision-dissipative instability of small gravity disturbances the disk is subdivided into numerous dense fragments. These can eventually condense into the planetary sequence.

引用

页码：181 / 183

页数：3