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Proceedings Paper

Infrared interferometric observations of T Tauri stars
Author(s): Rachel L. Akeson; David Ciardi; Gerard Theodore van Belle
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Paper Abstract

We present observations of several T Tauri stars using long baseline infrared interferometry from the Palomar Testbed Interferometer. The target sources, T Tau N, SU Aur, RY Tau and DR Tau, are all known to be surrounded by dusty circumstellar disks. The observations directly trace the inner regions (<1 AU) of the disk and can be used to constrain the physical properties of this material. For three of the sources observed, the size scale of the infrared emission is tenths of AU, which is considerably larger than predicted by flat disk models. We discuss the implications of these results for models of circumstellar material, in particular the recent theoretical work suggesting the presence of an extended vertical wall at the inner edge of the disk.

Paper Details

Date Published: 21 February 2003
PDF: 6 pages
Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); doi: 10.1117/12.457016
Show Author Affiliations
Rachel L. Akeson, California Institute of Technology (United States)
David Ciardi, Univ. of Florida (United States)
Gerard Theodore van Belle, Jet Propulsion Lab. (United States)


Published in SPIE Proceedings Vol. 4838:
Interferometry for Optical Astronomy II
Wesley A. Traub, Editor(s)

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