Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Radiative Transfer

Details Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Radiative Transfer Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Radiative Transfer

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1193b&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1193

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3

Scientific paper

Disk instability models including radiative transfer in the diffusion
approximation and detailed thermodynamics lead to the formation of
clumps similar to those in locally isothermal models, supporting the
hypothesis of gas giant protoplanet formation by this mechanism.

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