GIANT PLANET FORMATION ON WIDE ORBITS BY CORE ACCRETION

被引：0

作者：

Guilera, O. M. ^{[1
]}

Ronco, M. P. ^{[1
]}

机构：

[1] Inst Astrofis La Plata CONICET UNLP, Fac Ciencias Astron & Geofis UNLP, Grp Ciencias Planetarias, La Plata, Buenos Aires, Argentina

来源：

XV LATIN AMERICAN REGIONAL IAU MEETING, 2016 | 2017年 / 49卷

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 discovery of giant planets on wide orbits represents a major challenge for the standard core accretion model. In such model, giant planets are expected to form at small or moderate distances from the central star in order to form massive cores able to trigger the gaseous runaway growth before the dissipation of the disk. In this work, we present a new simple mechanism for the formation of giant planets on wide orbits by core accretion considering planet formation, planet migration and disk evolution.

引用

页码：73 / 73

页数：1

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