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DOI

10.20371/INAF/DS/2020_00003

Creators 
(name, orcid, 
affilation)
  • Ignazio Pillitteri: 0000-0003-4948-6550 - INAF-OAPa
Titles MHD simulation of a star with a hot Jupiter
Publisher  INAF - OAPa
Associated Paper Matsakos et al. (2015), Astronomy & Astrophysics, Volume 578, id.A6. 17pp.;
Pillitteri et al. (2015) ,The Astrophysical Journal, Volume 805, Issue 1, article id. 52, 18 pp.;
Mignone et al. The Astrophysical Journal Supplement Series, Volume 170, Issue 1, pp. 228-242. (2007);
Publication 2019
Resource type DataSet
Version 1.0
File .zip
Dimension 2.5 MB
description

 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).

rights

GNU GPL V3

link

MHD simulation of a star with a hot Jupiter