Could we identify hot ocean-planets with CoRoT, Kepler and Doppler velocimetry?
- 15 November 2007
- Vol. 191 (2) , 453-468
- https://doi.org/10.1016/j.icarus.2007.04.010
Abstract
No abstract availableKeywords
All Related Versions
This publication has 40 references indexed in Scilit:
- Formation and structure of the three Neptune-mass planets system around HD 69830Astronomy & Astrophysics, 2006
- The transmission spectrum of Earth-size transiting planetsAstronomy & Astrophysics, 2006
- Phase‐dependent Properties of Extrasolar Planet AtmospheresThe Astrophysical Journal, 2005
- Hot-Jupiters and hot-Neptunes: A common origin?Astronomy & Astrophysics, 2005
- Predicting accurate stellar angular diameters by the near-infrared surface brightness techniqueMonthly Notices of the Royal Astronomical Society, 2005
- TrES-1: The Transiting Planet of a Bright K0 V StarThe Astrophysical Journal, 2004
- The effect of evaporation on the evolution of close-in giant planetsAstronomy & Astrophysics, 2004
- Exoplanet detection capability of the COROT space missionAstronomy & Astrophysics, 2003
- Fundamental photon noise limit to radial velocity measurementsAstronomy & Astrophysics, 2001
- Hydrodynamic escape of hydrogen from a hot water‐rich atmosphere: The case of VenusJournal of Geophysical Research, 1996