Could we identify hot ocean-planets with CoRoT, Kepler and Doppler velocimetry?

Icarus

Volumn 191, Issue 2, 2007, Pages 453-468

  Selsis, F ^a   Chazelas, B ^b   Borde P ^c   Ollivier, M ^b   Brachet, F ^b   Decaudin, M ^b   Bouchy, F ^d   Ehrenreich, D ^d   Griessmeier J M ^e   Lammer, H ^f   Sotin, C ^g   Grasset, O ^g   Moutou, C ^h   Barge, P ^h   Deleuil, M ^h   Mawet, D ⁱ   Despois, D ^j   Kasting, J F ^k   Leger A ^b  

^a UNIVERSITÉ DE LYON   (France)

^b UNIVERSITÉ PARIS SACLAY   (France)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^e UNIVERSITÉ PARIS DIDEROT   (France)

^f Austrian Academy of Sciences ^*  (Austria)

^g UNIVERSITÉ DE NANTES   (France)

^h OBSERVATOIRE DE MARSEILLE   (France)

ⁱ UNIVERSITY OF LIÈGE   (Belgium)

^j STATION DE RADIOASTRONOMIE DE NANÇAY   (France)

^k PENNSYLVANIA STATE UNIVERSITY   (United States)

more..

Author keywords

Extrasolar planets; Ices; migration; Planets

Indexed keywords

EID: 35548985464     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2007.04.010     Document Type: Article

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