Detecting T Tauri disks with optical long-baseline interferometry

Details Detecting T Tauri disks with optical long-baseline interferometry Detecting T Tauri disks with optical long-baseline interferometry

1995-05-13

arxiv.org/abs/astro-ph/9505061v1

Astronomy and Astrophysics

Astrophysics

10 pages including figures and tables, uuencoded gz-compressed postscript; Accepted by Astronomy & Astrophysics Supplement Ser

Scientific paper

We present synthetic images of disks around T Tauri stars. We calculate visibility curves in order to study the possibility of directly detecting thermal emission from T Tauri disks. Total fluxes of T Tauri disks are compared to the sensitivity of VISA, the interferometric sub-array of the European Very Large Telescope. We conclude that thermal emission from circumstellar disk around T Tauri stars is detectable with current or soon-to-be interferometric techniques at wavelengths longer than 2.2 microns.

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