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New numerical models on giant planet formation

被引：0
|
作者：
Fortier, A.
Brunini, A.
Benvenuto, O. G.
机构：
来源：
XI IAU Regional Latin American Meeting of Astronomy | 2006年 / 26卷
关键词：
planets and satellites : formation;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present our results on giant planet formation in the frame of the nucleated instability mechanism. We consider the oligarchic growth regime for the solid core and a reduction in the grain opacity. Under these assumptions, in situ giant planet formation is achievable in a timescale shorter than the lifetime of protoplanetary disks.
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页码：3 / 4
页数：2
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