Protoplanets with core masses below the critical mass fill in their Roche lobe
We study the evolution of a protoplanet of a few earth masses embedded in a protoplanetary disc. If we assume that the atmosphere of the protoplanet, i.e. the volume of gas in hydrostatic equilibrium bound to the core, has a surface radius smaller than the Roche lobe radius, we show that it expands...
Main Authors: | Terquem, C, Heinemann, T |
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Format: | Journal article |
Language: | English |
Published: |
2011
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