Global evolution of solids in protoplanetary disks:: A simple model

被引：0
|
作者：
Rózyczka, M [1 ]
Kornet, K [1 ]
Bodenheimer, P [1 ]
Stepinski, T [1 ]
机构：
[1] Nicholas Copernicus Astron Ctr, Warsaw, Poland
来源：
GRAVITATIONAL COLLAPSE: FROM MASSIVE STARS TO PLANETS | 2004年 / 22卷
关键词：
accretion; accretion disks; stars : planetary systems : formation; stars : planetary systems : protoplanetary disks;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Various aspects of the evolution of solids in protoplanetary disks are discussed. While small bodies present in the disk grow in size, they decouple from the gas, resulting in a significant redistribution of solids within the disk. It is shown that the evolution of solids must be taken into account in models of planet formation via the core accretion - gas capture mechanism.
引用
收藏
页码：91 / 94
页数：4
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