Gas Dynamic Simulation of the Star-Planet Interaction using a Binary Star Model

被引：3

作者：

Ionov, D. E. ^{[1
]}

Bisikalo, D. V. ^{[1
]}

Kaygorodov, P. V. ^{[1
]}

Shematovich, V. I. ^{[1
]}

机构：

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

来源：

FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS | 2012年 / 282期

关键词：

planetary systems; binaries; hydrodynamics; MASS;

D O I：

10.1017/S1743921311028341

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have performed numerical simulations of the interaction between a "hot Jupiter" planet and gas of the stellar wind using a numerical code developed for investigations of binary stars. With this code, we have modeled the structure of the gaseous flow in the system HD 209458. The results have been used to explain observations of this system performed with the COS instrument on-board the HST.

引用

页码：545 / 546

页数：2

共 7 条

[1]

Bisikalo D. V., 2003, MATEMATICHESKOYE MOD, V71

[2] Morphology of the interaction between the stream and cool accretion disk in a semidetached binary system [J].