Segregation of heavy elements in an initial protoplanet
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Earth and Planetary Sciences
Link
https://link.springer.com/content/pdf/10.1007/s12145-020-00474-5.pdf
Reference35 articles.
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3. Boley AC, Hayfield T, Mayer L, Durisen RH (2010) Clumps in the outer disk by disk instability: why they are initially gas giants and the legacy of disruption. Icarus 207:509–516
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5. Boss AP (1998a) Evolution of the solar nebula. IV Giant gaseous protoplanet formation Astrophys J 503:923–937
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