The origin of hydrogen around HD 209458b

Nature

Volumn 456, Issue 7219, 2008, Pages

  Etangs, A Lecavelier Des ^a,b   Vidal Madjar, A ^a,b   Desert J M ^a,b  

^a INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^b SORBONNE UNIVERSITÉ   (France)

Author keywords

[No Author keywords available]

Indexed keywords

HYDROGEN;

ASTRONOMY; ATMOSPHERE; ATOM; NOTE; PRIORITY JOURNAL; RADIATION; SIMULATION;

EID: 56249136544     PISSN: 00280836     EISSN: 14764687     Source Type: Journal    
DOI: 10.1038/nature07402     Document Type: Note

References (4)

1. Holmström, M. et al. Energetic neutral atoms as the explanation for the high-velocity hydrogen around HD 209458b. Nature 451, 970-972 (2008).
2. Vidal-Madjar, A. et al. An extended upper atmosphere around the extrasolar planet HD209458b. Nature 422, 143-146 (2003).
3. Vidal-Madjar, A. et al. Exoplanet HD 209458b (Osiris). Evaporation strengthened. Astrophys. J. 676, L57-L60 (2008).
4. Vidal-Madjar, A. & Lecavelier des Etangs, A. "Osiris" (HD209458b), an Evaporating Planet. ASP Conf. Series 321, 152-159 (2004).