Paper:	Thermal Structure of Protoplanetary Disks
Volume:	341, Chondrites and the Protoplanetary Disk
Page:	353
Authors:	D'Alessio, P.; Calvet, N.; Woolum, D. S.
Abstract:	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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