New numerical models on giant planet formation

被引:0
|
作者
Fortier, A.
Brunini, A.
Benvenuto, O. G.
机构
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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