Growth of planetesimals and clearance of disks around the T-Tauri stars

Details Growth of planetesimals and clearance of disks around the T-Tauri stars Growth of planetesimals and clearance of disks around the T-Tauri stars

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988em%26p...43....1g&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 43, Oct. 1988, p. 1-6.

Physics

Accretion Disks, Cosmic Dust, Extrasolar Planets, Protoplanets, T Tauri Stars, Clearing, Condensation, Surface Properties

Scientific paper

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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