Modelling atmospheric escape and Mg ii near-ultraviolet absorption of the highly irradiated hot Jupiter WASP-12b-Reference-Cited by-同舟云学术

Modelling atmospheric escape and Mg ii near-ultraviolet absorption of the highly irradiated hot Jupiter WASP-12b

Published:2019-05-16 Issue:3 Volume:487 Page:4208-4220
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Dwivedi N K¹,Khodachenko M L¹²³,Shaikhislamov I F⁴,Fossati L¹,Lammer H¹,Sasunov Y¹²,Berezutskiy A G⁴,Miroshnichenko I B⁴,Kislyakova K G⁵,Johnstone C P⁵,Güdel M⁵

Affiliation:

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

2. Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119991 Moscow, Russia

3. Institute of Astronomy of the Russian Academy of Sciences, 119017 Moscow, Russia

4. Institute of Laser Physics SB RAS, Novosibirsk, RussiaInstitute of Laser Physics SB RAS, 630090 Novosibirsk, Russia

5. Department of Astrophysics, University of Vienna, A-1180 Vienna, Austria

Funder

Austrian Science Foundation

Austrian Agency for International Cooperation in Education and Research

Russian Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1345/28656761/stz1345.pdf

Reference56 articles.

1. Abundances of the elements: Meteoritic and solar

2. THREE-DIMENSIONAL GAS DYNAMIC SIMULATION OF THE INTERACTION BETWEEN THE EXOPLANET WASP-12b AND ITS HOST STAR

3. The maximum size of a stationary, quasi-closed gaseous envelope around the hot jupiter WASP-12b

4. 3D model of hydrogen atmospheric escape from HD 209458b and HD 189733b: radiative blow-out and stellar wind interactions

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