Distribution of thermodynamic variables inside extra-solar protoplanets formed via disk instability
Author:
Publisher
Elsevier BV
Subject
General Earth and Planetary Sciences
Reference21 articles.
1. The internal energy for molecular hydrogen in gravitationally unstable protoplanetary disks;Boley;Astrophys. J.,2007
2. Erratum: “the internal energy for molecular hydrogen in gravitationally unstable protoplanetary disks”;Boley;Astrophys. J.,2007
3. Clumps in the outer disk by disk instability: why they are initially gas giants and the legacy of disruption;Boley;Icarus,2010
4. Giant planet formation by gravitational instability;Boss;Science,1997
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