The evolution of protoplanetary disks

Details The evolution of protoplanetary disks The evolution of protoplanetary disks

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...36..197r&link_type=abstract

In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36

Physics

13

Accretion Disks, Planetary Evolution, Planetary Systems, Pulsars, Stellar Evolution, Angular Momentum, Extrasolar Planets, Momentum Transfer

Scientific paper

Accretion disks evolve by transferring angular momentum outwards, which allows mass to flow inwards onto the central object. The radial structure and time-dependent behavior of low-mass, Keplerian, viscous disks is analyzed. Potential mechanisms for the angular momentum transport in disks are reviewed. An evolutionary model of a low mass disk around a pulsar is presented.

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