The effects of self-gravity on the solar nebula

Details The effects of self-gravity on the solar nebula The effects of self-gravity on the solar nebula

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..515y&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

1

Accretion Disks, Angular Momentum, Gravitational Effects, Momentum Transfer, Protostars, Solar System, Stellar Mass Accretion, Density Wave Model, Gravitational Collapse, Rotating Fluids, Solar Rotation, Stellar Evolution

Scientific paper

The distribution and transport of angular momentum in a self-gravitating accretion disk formed during the collapse of a rotating gas cloud has been studied. Using the surface density for the low-viscosity models and minimum-mass models presented by Cassen and Summers (1983), Poisson's equation is solved explicitly to determine the effects of self-gravitation of the protostellar disk. Analytic expressions for the angular momentum of the central star and other relevant quantities of interest during the formation stage are presented.

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