Orbital migration induced by anisotropic evaporation Can hot Jupiters form hot Neptunes?

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Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 537; p. L3
Main Authors Boué, G., Figueira, P., Correia, A. C. M., Santos, N. C.
Format Journal Article
LanguageEnglish
Published Les Ulis EDP Sciences 01.01.2012
Subjects
Astronomy
Astrophysics
Earth, ocean, space
Exact sciences and technology
Physics
Energetics
Extrasolar planets
planets and satellites: dynamical evolution and stability
Mass loss
Probability
Orbits
Evaporation
planet-star interactions
Jupiter planet
Planetary cosmogony
Dynamical evolution
Neptune planet
Dynamic stability
planets and satellites: formation
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More Information
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/201118084