A two-layer circumstellar disc model: interpreting spectra and visibilities

Details A two-layer circumstellar disc model: interpreting spectra and visibilities A two-layer circumstellar disc model: interpreting spectra and visibilities

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..457l&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present an analytical T Tauri disk model including viscous heating, stellar light reprocessing and thermalization with the surrounding medium. It is fast to compute, compares well with numerical simulations available in the literature, and allows, for the first time, to explain consistently both spectra and optical visibilities for young stellar object. It shall therefore be an ideal tool for model-fitting of large sets of data that new interferometers will provide.

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