ACS Coronagraphic Search for Debris Disks around Solar-type Stars

Physics

Scientific paper

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Scientific paper

This ACS/GTO program will image 5 nearby, A & G type stars to detect scattered light from circumstellar disks. These stars have significant infrared excesses that suggest that they are surrounded by dust that may be visible at the contrast level afforded by the ACS HRC coronagraph. One star, HD 32297, has a disk that has been imaged from the ground and by NICMOS.

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