Dust Around First Ascent Red Giants

Physics

Scientific paper

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Scientific paper

We propose to use MIPS to measure the dust around first ascent red giants which show infrared excesses in the IRAS data base. Our goal is to infer the mass, spatial distribution and temperature of the particles with the hope of inferring their origin. We chose stars that lie within 150 pc of the Sun that display an excess at 60 microns of at least 0.5 Jy and lie at absolute Galactic latitude greater than 10.

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