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- W2090205023 endingPage "120" @default.
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- W2090205023 abstract "We present the novel concept of evaporation of planetesimals as a result of bow shocks associated with planetesimals orbiting with supersonic velocities relative to the gas in a protoplanetary disk. We evaluate the evaporation rates of the planetesimals based on a simple model describing planetesimal heating and evaporation by the bow shock. We find that icy planetesimals with radius {approx}>100 km evaporate efficiently even outside the snow line in the stage of planetary oligarchic growth, where strong bow shocks are produced by gravitational perturbations from protoplanets. The obtained results suggest that the formation of gas giant planets is suppressed owing to insufficient accretion of icy planetesimals onto the protoplanet within the {approx}<5 AU disk region." @default.
- W2090205023 created "2016-06-24" @default.
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- W2090205023 date "2013-01-30" @default.
- W2090205023 modified "2023-09-25" @default.
- W2090205023 title "EVAPORATION OF ICY PLANETESIMALS DUE TO BOW SHOCKS" @default.
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- W2090205023 doi "https://doi.org/10.1088/0004-637x/764/2/120" @default.
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