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Planets and Satellites: Individual: Hd 189733b
A chemical model for the atmosphere of hot Jupiters
Context. The atmosphere of hot Jupiters can be probed by primary transit and secondary eclipse spectroscopy. Owing to the intense UV …
O. Venot
,
E. Hébrard
,
M. Agúndez
,
M. Dobrijevic
,
F. Selsis
,
F. Hersant
,
N. Iro
,
R. Bounaceur
Posted Oct 1, 2012
Cite
DOI
arXiv