An analytical model for the evolution of an accretion protoplanetary disk

Details An analytical model for the evolution of an accretion protoplanetary disk An analytical model for the evolution of an accretion protoplanetary disk

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989avest..23..125g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 23, Apr.-June 1989, p. 125-133. In Russian.

Statistics

Computation

Accretion Disks, Astronomical Models, Planetary Evolution, Protoplanets, Angular Momentum, Computational Astrophysics, Solar System

Scientific paper

An analytical model for the evolution of a protoplanetary disk is developed under conditions of direct accretion of matter onto it. The model is constructed in the approximation of small angular momentum (J of about 10 to the 52nd g sq cm/s). It is shown that the resulting evolutionary scenario is qualitatively different from the case in which the accretion of matter on the disk was not considered.

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