Post-main-sequence planetary system evolution

被引：178
|
作者：
Veras, Dimitri [1 ]
机构：
[1] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
来源：
ROYAL SOCIETY OPEN SCIENCE | 2016年 / 3卷 / 02期
关键词：
dynamics; white dwarfs; giant branch stars; pulsars; asteroids; formation; ASYMPTOTIC GIANT BRANCH; PRECISE RADIAL-VELOCITIES; EXCESS INFRARED RADIATION; NEUTRON-STAR ACCRETION; COMPACT DEBRIS DISKS; SINGLE WHITE-DWARFS; FINAL MASS RELATION; N-BODY SIMULATIONS; BROWN DWARFS; STELLAR EVOLUTION;
D O I：
10.1098/rsos.150571
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical scrutiny. Here, I review the diverse dynamical processes which affect planets, asteroids, comets and pebbles as their parent stars evolve into giant branch, white dwarf and neutron stars. This reference provides a foundation for the interpretation and modelling of currently known systems and upcoming discoveries.
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页数：65
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