Planetary systems in dense stellar environments

Author:

Kouwenhoven M B N,Flammini Dotti Francesco,Shu Qi,Xu Xiuming,Wu Kai,Pang Xiaoying,Hao Wei

Abstract

Abstract The recent advances in observational and computational techniques allow studying the formation and dynamical evolution of planetary systems at an unprecedented level. The formation and evolution of isolated planetary systems are challenging in itself and it is more complicated by the dense environments in which stars and planets are typically born. Here, we present an overview of the internal and external processes that govern the dynamical evolution of planetary systems, and we provide a brief overview of a selection of the computational tools that are presently available to carry out realistic simulations of planetary systems in dense stellar environments.

Publisher

IOP Publishing

Subject

General Physics and Astronomy

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The dynamical evolution of protoplanetary discs and planets in dense star clusters;Monthly Notices of the Royal Astronomical Society;2023-09-18

2. Computational methods for collisional stellar systems;Living Reviews in Computational Astrophysics;2023-09-06

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