Detecting T Tauri disks with optical long-baseline interferometry

F. Malbet; C. Bertout

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arXiv · astro-ph/9505061

Detecting T Tauri disks with optical long-baseline interferometry

F. Malbet·C. Bertout

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Abstract

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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F. Malbet, C. Bertout. 1995-05-13. Detecting T Tauri disks with optical long-baseline interferometry. https://arxiv.org/abs/astro-ph/9505061

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