The clearing of planetesimal disks around T Tauri type stars

Details The clearing of planetesimal disks around T Tauri type stars The clearing of planetesimal disks around T Tauri type stars

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22..319g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, Oct.-Dec. 1988, p. 319-325. In Russian.

Astronomy and Astrophysics

Astronomy

Cosmic Dust, Planetary Nebulae, Protoplanets, Stellar Evolution, T Tauri Stars, Disks (Shapes), Early Stars, Optical Thickness

Scientific paper

The growth and collapse of dust condensations formed as a result of the development of gravitational instability in a dusty subdisk are discussed within the framework of a generally accepted scenario for the evolution of a circumsolar protoplanetary disk. The time of enlargment of the condensations required for clearing the hypothetical disks around young solar-type stars is estimated.

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