Gas accretion by planetary cores
classification
🌌 astro-ph.EP
keywords
accretionratescoresmassmodelscoredependencefound
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We present accretion rates obtained from three-dimensional self-gravitating radiation hydrodynamical models of giant planet growth. We investigate the dependence of accretion rates upon grain opacity and core/protoplanet mass. The accretion rates found for low mass cores are inline with the results of previous one-dimensional models that include radiative transfer.
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