MHD simulation of a star with a hot Jupiter
收藏DataCite Commons2024-08-07 更新2024-07-13 收录
下载链接：
https://openscience.inaf.it/?page_id=481
下载链接
链接失效反馈官方服务：
资源简介：
The scene shows a frame of an MHD simulation of a system formed by a K type star and a planet the size of Jupiter.
The simulation is made with PLUTO code (Mignone et al., 2007). Given the short separation, the atmosphere of the planet
is evaporating and forms a tail behind the planet. Furthermore, part of the gas is launched towards the star
and precipitates on it. The work is based on Matsakos et al. (2015) and Pillitteri et al. (2015).
提供机构：
INAF-OAPa
创建时间：
2020-10-06
