Observational Constraints on Transport (and Mixing) in Pre-Main Sequence Disks

Details Observational Constraints on Transport (and Mixing) in Pre-Main Sequence Disks Observational Constraints on Transport (and Mixing) in Pre-Main Sequence Disks

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ssrv...92...55h&link_type=abstract

Space Science Reviews, v. 92, Issue 1/2, p. 55-68 (2000).

Physics

10

Scientific paper

Currently available observational constraints on transport mechanisms in
pre-main sequence disks are reviewed. The main observable quantity
accessable by imaging the spatial structure of disks is the mass
accretion rate, which constrains angular momentum transport, and
migration and diffusion of disk material.

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