Protoplanetary disks: Observations and physical processes

Details Protoplanetary disks: Observations and physical processes Protoplanetary disks: Observations and physical processes

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.315..219m&link_type=abstract

In ESA, Formation of Stars and Planets and the Evolution of the Solar System p 219-227 (SEE N91-18922 10-90)

Astronomy and Astrophysics

Astronomy

4

Accretion Disks, Astronomical Models, Planetary Evolution, Protoplanets, Electrical Properties, Planetary Environments, Planetary Mass, Stellar Evolution

Scientific paper

Observations of disks around young premain stars are reviewed. A summary of disk properties is presented. The disks are the most likely environment for planet formation. The observations are interpreted in the context of steady accretion disk models. Observed departures from such a standard model are discussed in terms of different physical processes as well as time dependence. The processes leading to electrical discharges in the protoplanetary disk are described.

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