Supermassive hot Jupiters provide more favourable conditions for the generation of radio emission via the cyclotron maser instability – a case study based on Tau Bootis b-Reference-Cited by-同舟云学术

Supermassive hot Jupiters provide more favourable conditions for the generation of radio emission via the cyclotron maser instability – a case study based on Tau Bootis b

Published:2018-08-01 Issue:3 Volume:480 Page:3680-3688
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Weber C¹²^ORCID,Erkaev N V³⁴,Ivanov V A⁴,Odert P¹⁵,Grießmeier J-M⁶⁷,Fossati L¹,Lammer H¹,Rucker H O⁸

Affiliation:

1. Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, A-8042 Graz, Austria

2. Institute of Atmospheric Physics, Czech Academy of Sciences, CZ-141 31 Prague, Czech Republic

3. Institute of Computational Modelling SB RAS, 660036, Krasnoyarsk, 6Russian Federation

4. Siberian Federal University, 660041 Krasnoyarsk, Russian Federation

5. Institute of Physics/IGAM, University of Graz, Universitätsplatz 5, A-8010 Graz, Austria

6. LPC2E - Université d’Orléans/CNRS, F-45071Orléans, France

7. Station de Radioastronomie de Nançay, Observatoire de Paris, PSL Research University, CNRS/INSU, USR 704 - Univ. Orléans, OSUC, route de Souesmes, 18330 Nançay, France

8. Comm. Astron., Austrian Academy of Sciences, A-8042 Graz, Austria

Funder

Austrian Science Fund

Russian Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/3/3680/25519279/sty2079.pdf

Reference70 articles.

1. A Search for Radio Emission from Extrasolar Planets