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- W2953262362 abstract "The kinetic theory is used to study the evolution of the self-gravitating disk of planetesimals. The effects of frequent collisions between planetesimals are taken into account by using a Krook integral in the Boltzmann kinetic equation. It is shown that as a result of an aperiodic collision-dissipative instability of small gravity disturbances the disk is subdivided into numerous dense fragments. These can eventually condense into the planetary sequence." @default.
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- W2953262362 date "2000-12-05" @default.
- W2953262362 modified "2023-10-16" @default.
- W2953262362 title "Formation of the Planetary Sequence in a Highly Flattened Disk of Frequently Colliding Planetesimals" @default.
- W2953262362 doi "https://doi.org/10.48550/arxiv.astro-ph/0012101" @default.
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