Growth of planetesimals and clearance of disks around the T-tauri stars |
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| Authors: | K. M. Guseinov |
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| Affiliation: | (1) O. Yu. Schmidt Institute of Physics of the Earth, Academy of Sciences of the USSR, Moscow, U.S.S.R. |
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| Abstract: | A growth and contraction of dust condensations formed as a result of development of gravitation instability in a dust subdisk is discussed within the framework of the generally accepted scheme of evolution of a circumsolar pre-planetary disk. The time of evolution of condensations necessary for clearing the hypothetical disks around young stars of the Sun type is estimated. |
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