Тип публикации: статья из журнала

Год издания: 2018

Идентификатор DOI: 10.1093/MNRAS/STY2079

Аннотация: We investigate under which conditions supermassive hot Jupiters can sustain source regions for radio emission, and whether this emission could propagate to an observer outside the system. We study Tau Bootis b-like planets (a supermassive hot Jupiter with

Журнал: Monthly Notices of the Royal Astronomical Society

Выпуск журнала: Vol. 480, Is. 3

Номера страниц: 3680-3688

ISSN журнала: 00358711

Издатель: Oxford University Press

• Weber C. (Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria; Czech Acad Sci, Inst Atmospher Phys, CZ-14131 Prague, Czech Republic)
• Erkaev N.V. (Inst Computat Modelling SB RAS, Krasnoyarsk 660036, Russia; Siberian Fed Univ, Krasnoyarsk 660041, Russia)
• Ivanov V.A. (Siberian Fed Univ, Krasnoyarsk 660041, Russia)
• Odert P. (Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria; Karl Franzens Univ Graz, Inst Phys IGAM, Univ Pl 5, A-8010 Graz, Austria)
• Griessmeier J.-M. (Univ Orleans, CNRS, LPC2E, F-45071 Orleans, France; PSL Res Univ, CNRS INSU, USR 704 Univ Orleans, Stn Radioastron Nancay,Observ Paris,OSUC, Route Souesmes, F-18330 Nancay, France)
• Fossati L. (Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria)
• Lammer H. (Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria)
• Rucker H.O. (Austrian Acad Sci, Comm Astron, A-8042 Graz, Austria)

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