The formation of planetary systems during the evolution of close binary stars

Details The formation of planetary systems during the evolution of close binary stars The formation of planetary systems during the evolution of close binary stars

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..837t&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, July-Aug. 1991, p. 837-842. In Russian.

Astronomy and Astrophysics

Astronomy

4

Binary Stars, Planetary Systems, Stellar Evolution, Cosmic Dust, Cosmology, Stellar Mass Accretion

Scientific paper

Modern scenarios of the formation of planetary systems around single stars and products of merging close binaries are described. The frequencies of the realization of different scenarios in the Galaxy are estimated. It is concluded that the modern theory of the early stages of the evolution of single stars and the theory of the evolution of close binaries offer several possible versions for the origin of planetary systems, while the scenario dating back to Kant and Laplace remains the likeliest.

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