Тип публикации: статья из журнала

Год издания: 2018

Идентификатор DOI: 10.3847/1538-4357/aadf39

Ключевые слова: hydrodynamics, planet-star interactions, planets and satellites: atmosphere, planets and satellites: individual (exoplanets), planets and satellites: physical evolution, plasmas

Аннотация: The absorption of stellar radiation observed by HD 209458b in the resonant lines of O I and C II has not yet been satisfactorily explained. We apply a 2D hydrodynamic multi-fluid model that self-consistently describes the expanding planetary wind, driven

Журнал: ASTROPHYSICAL JOURNAL

Выпуск журнала: Vol. 866, Is. 1

Номера страниц: 47

ISSN журнала: 0004637X

Место издания: BRISTOL

Издатель: IOP PUBLISHING LTD

• Shaikhislamov I.F. (Inst Laser Phys SB RAS, Novosibirsk, Russia)
• Khodachenko M.L. (Austrian Acad Sci, Space Res Inst, Graz, Austria; Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia)
• Lammer H. (Austrian Acad Sci, Space Res Inst, Graz, Austria)
• Fossati L. (Austrian Acad Sci, Space Res Inst, Graz, Austria)
• Dwivedi N. (Austrian Acad Sci, Space Res Inst, Graz, Austria)
• Guedel M. (Univ Vienna, Dept Astrophys, Vienna, Austria)
• Kislyakova K.G. (Austrian Acad Sci, Space Res Inst, Graz, Austria; Univ Vienna, Dept Astrophys, Vienna, Austria)
• Johnstone C.P. (Univ Vienna, Dept Astrophys, Vienna, Austria)
• Berezutsky A.G. (Inst Laser Phys SB RAS, Novosibirsk, Russia)
• Miroshnichenko I.B. (Inst Laser Phys SB RAS, Novosibirsk, Russia)
• Posukh V.G. (Inst Laser Phys SB RAS, Novosibirsk, Russia)
• Erkaev N.V (Inst Computat Modelling SB RAS, Krasnoyarsk, Russia; Siberian Fed Univ, Polytech Inst, Krasnoyarsk, Russia)
• Ivanov V.A. (Siberian Fed Univ, Polytech Inst, Krasnoyarsk, Russia)

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