Detecting T Tauri disks with optical long-baseline interferometry

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dc.creatorMalbet, F.
dc.creatorBertout, C.
dc.date1995-05-13
dc.date.accessioned2026-07-07T02:19:46Z
dc.date.available2026-07-07T02:19:46Z
dc.descriptionWe 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.
dc.description10 pages including figures and tables, uuencoded gz-compressed postscript; Accepted by Astronomy & Astrophysics Supplement Series
dc.identifierhttps://arxiv.org/abs/astro-ph/9505061
dc.identifierhttp://arxiv.org/abs/astro-ph/9505061
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10000
dc.subjectAstrophysics
dc.titleDetecting T Tauri disks with optical long-baseline interferometry
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