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JOURNALS // Preprints of the Keldysh Institute of Applied Mathematics // Archive

Keldysh Institute preprints, 2018 229, 31 pp. (Mi ipmp2587)

This article is cited in 6 papers

To the question of the formation model of planetary systems of stars

M. S. Legkostupov


Abstract: The model of the formation of planetary systems of stars is presented, which is based on the origin and development of large-scale gravitational instabilities (protoplanetary rings) in a protoplanetary disk.

Keywords: protosolar nebular, collapse, protoplanetary gas-dust disk, gravitational instability, protoplanetary gas-dust ring, planetary system.

DOI: 10.20948/prepr-2018-229



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© Steklov Math. Inst. of RAS, 2026