Model protoplanetary disks around F-G stars

Details Model protoplanetary disks around F-G stars Model protoplanetary disks around F-G stars

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..371v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, June 1982, p. 371-377.) Soviet Astronomy Letters, vol. 8, May-June 1982, p. 201-205.

Astronomy and Astrophysics

Astronomy

Accretion Disks, F Stars, G Stars, Main Sequence Stars, Planetary Evolution, Protoplanets, Stellar Models, Angular Momentum, Cosmic Dust, Disks (Shapes), Interstellar Gas

Scientific paper

Some topics in the formation and early evolution of protoplanetary gas-dust disks around single solar-type stars are discussed. A new class of disk models is proposed, whose parameters are the disk mass and angular momentum as well as the mass and luminosity of the central star. Since disks may persist for fully 10 to the 8th yr, a search for them among the members of decaying clusters would be worthwhile

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