Exoplanet HD 209458b (Osiris): Evaporation Strengthened-Reference-Cited by-同舟云学术

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Exoplanet HD 209458b (Osiris): Evaporation Strengthened

Published:2008-03-04 Issue:1 Volume:676 Page:L57-L60
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Vidal-Madjar A.,Lecavelier des Etangs A.,Désert J.-M.,Ballester G. E.,Ferlet R.,Hébrard G.,Mayor M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference19 articles.

1. The signature of hot hydrogen in the atmosphere of the extrasolar planet HD 209458b

2. Hot-Jupiters and hot-Neptunes: A common origin?

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

4. Detection of an Extrasolar Planet Atmosphere

5. Physical and chemical aeronomy of HD 209458b

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1. The Mass Fractionation of Helium in the Escaping Atmosphere of HD 209458b*;The Astrophysical Journal;2023-08-01

2. 3D Numerical Model of the Envelope of a Hot Exoplanet Based on Spherical Coordinates;Astronomy Reports;2023-04

3. 3D Numerical Model of the Envelope of a Hot Exoplanet Based on Spherical Coordinates;Астрономический журнал;2023-04-01

4. The Hubble PanCET program: The near-ultraviolet transmission spectrum of WASP-79b;Astronomy & Astrophysics;2023-03-28

5. The Hubble/STIS near-ultraviolet transmission spectrum of HD 189733 b;Astronomy & Astrophysics;2023-03

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