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

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Boue G ^a,b   Figueira, P ^a   Correia, A C M ^b,c   Santos, N C ^a,d  

^a CENTRO DE ASTROFÍSICA   (Portugal)

^b Institut de Mecanique Celeste et de Calcul des ephemerides   (France)

^c UNIVERSITY OF AVEIRO   (Portugal)

^d UNIVERSITY OF PORTO   (Portugal)

Author keywords

Planet star interactions; Planets and satellites: dynamical evolution and stability; Planets and satellites: formation

Indexed keywords

ANALYTICAL RESULTS; ATMOSPHERIC MASS LOSS; EXO-PLANETS; JUPITERS; MASS EJECTION; ORBITAL EVOLUTIONS; ORBITAL MIGRATION; ORBITAL PERIODS; PLANET SURFACE; PLANETS AND SATELLITES: FORMATION;

EVAPORATION; INTERPLANETARY FLIGHT; PHASE TRANSITIONS; PLANETS; POPULATION DISTRIBUTION; PROBABILITY DISTRIBUTIONS; STARS;

SATELLITES;

EID: 84855369263     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118084     Document Type: Article

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