TWO REGIMES OF INTERACTION OF A HOT JUPITER’S ESCAPING ATMOSPHERE WITH THE STELLAR WIND AND GENERATION OF ENERGIZED ATOMIC HYDROGEN CORONA-Reference-Cited by-同舟云学术

TWO REGIMES OF INTERACTION OF A HOT JUPITER’S ESCAPING ATMOSPHERE WITH THE STELLAR WIND AND GENERATION OF ENERGIZED ATOMIC HYDROGEN CORONA

Published:2016-11-30 Issue:2 Volume:832 Page:173
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Shaikhislamov I. F.,Khodachenko M. L.^ORCID,Lammer H.,Kislyakova K. G.^ORCID,Fossati L.^ORCID,Johnstone C. P.^ORCID,Prokopov P. A.,Berezutsky A. G.,Zakharov Yu. P.,Posukh V. G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/832/i=2/a=173/pdf

Reference57 articles.

1. Exoplanet HD 209458b: Inflated Hydrogen Atmosphere but No Sign of Evaporation

2. Spectral, Spatial, and Time Properties of the Hydrogen Nebula around Exoplanet HD 209458b

3. ON THE EXISTENCE OF ENERGETIC ATOMS IN THE UPPER ATMOSPHERE OF EXOPLANET HD209458b

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

5. Radiative braking in the extended exosphere of GJ 436 b

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