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...

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Bibliographic Details
Main Authors: Terquem, C, Heinemann, T
Format: Journal article
Language:English
Published: 2011

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