Thermal Structure of Protoplanetary Disks

Details Thermal Structure of Protoplanetary Disks Thermal Structure of Protoplanetary Disks

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..341..353d&link_type=abstract

Chondrites and the Protoplanetary Disk, ASP Conference Series, Vol. 341, Proceedings of a workshop held 8-11 November 2004 in Ka

Astronomy and Astrophysics

Astronomy

11

Scientific paper

We discuss results of the thermal structure of models of steady accretion disks, irradiated by their central stars, in which dust sublimation, growth and settling is taken into account self-consistently. The models are constrained by comparison with different observations of Classical T Tauri Stars with ages between 1 and 10 million years. The implications of these models for the interpretation of planetary data is also discussed.

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