Formation of planets during the evolution of single and binary stars

被引：26

作者：

Tutukov, A. V. ^{[1
,2
]}

Fedorova, A. V. ^{[1
,2
]}

机构：

[1] Russian Acad Sci, Inst Astron, Moscow, Russia

[2] Russian Acad Sci, Inst Astron, Moscow V71, Russia

来源：

ASTRONOMY REPORTS | 2012年 / 56卷 / 04期

基金：

俄罗斯基础研究基金会;

关键词：

INTERGALACTIC STARS; ANGULAR-MOMENTUM; MASS; CLUSTER; SYSTEM; COMPANIONS; DISCOVERY; FREQUENCY; SEARCH; ORBIT;

D O I：

10.1134/S1063772912040075

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Current views of the origin and evolution of single and binary stars suggest that the planets can form aroundmain-sequence single and binary stars, degenerate dwarfs, neutron stars, and stellarmass black holes according to several scenarios. Planets can arise during the formation of a star mainly due to excess angular momentum leading to the formation of an accretion-decretion disk of gas and dust around a single star or the components of a binary. It is the evolution of such disks that gives rise to planetary systems. A disk can arise around a star during its evolution due to the accretion of matter from dense interstellar clouds of gas and dust onto the star, the accretion of mass froma companion in a binary system, and the loss of matter during the contraction of a rapidly rotating star, in particular, if the star rotates as a rigid body and the rotation accelerates with its evolution along the main sequence. The fraction of stars with planetary systems is theoretically estimated as 30-40%, which is close to the current observational estimate of similar to 34%.

引用

页码：305 / 314

页数：10

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