Constraining T-Tauri disk models with interferometric measurements

Details Constraining T-Tauri disk models with interferometric measurements Constraining T-Tauri disk models with interferometric measurements

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..211l&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

Past observations of circumstellar disks (imaging and SED) are poor constraints for models of the inner regions. Together with F. Malbet and J.-L. Monin I developped a model of T Tauri disks. I shall use these models to show what we can expect from present or soon-to-be interferometric techniques. Recent interferometric observations showed that disks can be resolved with baselines of 10 to 100 meters. In the near future we want to take advantage of the new instruments: - interferometry with more than 2 telescopes allows to determine the inclination of the disk and discard the presence of a binary - closure phase measurments give us the asymmetry of the distribution, thence we can determine the flaring of the disk

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