Gas accretion by planetary cores

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

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To be published in American Institute of Physics; Conference proceedings - Exoplanets and Disks: Their Formation and Diversity

Scientific paper

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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