Theory of Protoplanetary Disks

Details Theory of Protoplanetary Disks Theory of Protoplanetary Disks

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.223...57r&link_type=abstract

Astrophysics and Space Science, Volume 223, Issue 1-2, pp. 57-68

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The evolution of protoplanetary disks around young stars is briefly
reviewed. The most important physical mechanisms that drive the mass
accretion are gravitational, magnetic, and thermal convective
instabilities. These mechanisms are dominant in different regions of the
disk and at different evolutionary epochs.

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