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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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