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

• Published in: Astronomy and astrophysics (Berlin) Vol. 537; p. L3
• Main Authors: Boué, G., Figueira, P., Correia, A. C. M., Santos, N. C.
• Format: Journal Article
• Language: English
• 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