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.

引用

页码：3 / 4

页数：2

共 5 条

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