Near-Infrared Coronagraphic Observations of the T Tauri Binary System UY Aur

Details Near-Infrared Coronagraphic Observations of the T Tauri Binary System UY Aur Near-Infrared Coronagraphic Observations of the T Tauri Binary System UY Aur

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lyot.confe..46h&link_type=abstract

Proceedings of the conference In the Spirit of Bernard Lyot: The Direct Detection of Planets and Circumstellar Disks in the 21s

Physics

Optics

Scientific paper

We obtained high resolution (~0.1) near-infrared images of UY Aur using the Coronagraphic Imager with Adaptive Optics (CIAO) on the Subaru Telescope. UY Aur is classical T Tauri binary systems. We detected a half-ring shaped circumbinary disk around UY Aur. It has a clumpy structure along the disk and a cavity between the binary and the disk. The lower limit of the clump mass is calculated to be ~9.6 earth mass, assuming optically thin conditions in near-infrared.

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