Planetary systems formation and the diversity of extrasolar systems

被引：0

作者：

Miguel, Yamila ^{[1
]}

Guilera, Octavio M. ^{[1
]}

Brunini, Adrian ^{[1
]}

机构：

[1] Univ Nacl La Plata, Fac Cs Astron & Geofis, La Plata, Buenos Aires, Argentina

来源：

ASTROPHYSICS OF PLANETARY SYSTEMS: FORMATION, STRUCTURE, AND DYNAMICAL EVOLUTION | 2011年 / 276期

关键词：

planets and satellites: formation; planetary systems: formation; ACCRETION;

D O I：

10.1017/S1743921311020710

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

With the end of answer questions as, how common are planetary systems like our own in the Universe? and What is the diversity of planetary systems that we could find in the universe?, we develop a semi-analytical model for computing planetary systems formation and consider different initial conditions for generating a large sample of planetary systems, which is analysed statistically. We explore the effects in the planetary system architecture of assuming different initial disc profiles and planetary migration rates.

引用

页码：441 / 442

页数：2

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