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• W2165728884 abstract "The observed mass function for all known extrasolar giant planets (EGPs) varies approximately as M-1 for mass M between ~0.2 Jupiter masses (MJ) and ~5 MJ. In order to study evaporation effects for highly irradiated EGPs in this mass range, we have constructed an observational mass function for a subset of EGPs in the same mass range but with orbital radii <0.07 AU. Surprisingly, the mass function for such highly irradiated EGPs agrees quantitatively with the M-1 law, implying that the mass function for EGPs is preserved despite migration to small orbital radii. Unless there is a remarkable compensation of mass-dependent orbital migration for mass-dependent evaporation, this result places a constraint on orbital migration models and rules out the most extreme mass-loss rates in the literature. A theory that predicts more moderate mass loss gives a mass function that is closer to observed statistics but still disagrees for M < 1 MJ." @default.
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• W2165728884 date "2007-02-16" @default.
• W2165728884 modified "2023-09-26" @default.
• W2165728884 title "A Mass Function Constraint on Extrasolar Giant Planet Evaporation Rates" @default.
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• W2165728884 doi "https://doi.org/10.1086/513422" @default.
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