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Stars are presented which have characteristics similar to Vega and other main-sequence stars with cool dust disks, based on the IRAS Point Source Catalog fluxes. The objects are selected to have a 60 |xm/100 |xm ratio similar to Vega, ß Pic, a PsA, and e Eri, and they are also required to show evidence of extension in the IRAS Working Survey Database. The fluxes are modeled using a blackbody energy distribution. The temperatures derived range from 50 K to 650 K. The diameters of the dust disks observed by IRAS are estimated.

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