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Multi-component MHD model for hydrogen-helium extended envelope of hot Jupiter

Published online by Cambridge University Press:  20 January 2023

Y.G. Gladysheva
Affiliation:
Institute of Astronomy of the Russian Academy of Sciences, 48 Pyatnitskaya st. 119017, Moscow, Russia email: ygladysheva@inasan.ru
A.G. Zhilkin
Affiliation:
Institute of Astronomy of the Russian Academy of Sciences, 48 Pyatnitskaya st. 119017, Moscow, Russia email: ygladysheva@inasan.ru
D.V. Bisikalo
Affiliation:
Institute of Astronomy of the Russian Academy of Sciences, 48 Pyatnitskaya st. 119017, Moscow, Russia email: ygladysheva@inasan.ru
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Abstract

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We describe a numerical model of hot Jupiter extended envelope that interacts with stellar wind. Our model is based on approximation of multi-component magnetic hydrodynamic. The processes of ionization, recombination, dissosiation and chemical reactions in hydrogen-helium envelope are taken into account. In particular, the ionization of neutral hydrogen atoms takes place due to processes of photo-ionization, charge-exchange and thermal collisions. Further, this model is supposed to be used for research on biomarkers’ dynamics in extended envelopes of hot Jupiters.

Type
Poster Paper
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Zhilkin, A.G., & Bisikalo, D.V. 2021, Universe, 7, 422 CrossRefGoogle Scholar
Shaikhislamov, I.F., Khodachenko, M.L., Lammer, H., Kislyakova, K.G., Fossati, L., Johnstone, C.P., Prokopov, P.A., Berezutsky, A.G., Zakharov, Yu.P., & Posukh, V. G. 2016, Nature, 173, 20 Google Scholar
McElroy, D., Walsh, C., Markwick, A.J., Cordiner, M.A., Smith, K., & Millar, T.J. 2019, A&A, 550, 13 Google Scholar