WIRED for EC: New White Dwarfs with $\text{WISE}$ Infrared Excesses and New Classification Schemes from the Edinburgh-Cape Blue Object Survey

Abstract

We present a simple method for identifying candidate white dwarf systems with dusty exoplanetary debris based on a single temperature blackbody model fit to the infrared excess. We apply this technique to a sample of Southern Hemisphere white dwarfs from the recently completed Edinburgh-Cape Blue Object Survey and identify four new promising dusty debris disk candidates. We demonstrate the efficacy of our selection method by recovering three of the four $\text{Spitzer}$ confirmed dusty debris disk systems in our sample. Further investigation using archival high resolution imaging shows $\text{Spitzer}$ data of the un-recovered fourth object is likely contaminated by a line-of-sight object that either led to a mis-classification as a dusty disk in the literature or is confounding our method. Finally, in our diagnostic plot we show that dusty white dwarfs which also host gaseous debris lie along a boundary of our dusty debris disk region, providing clues to the origin and evolution of these especially interesting systems.

21 pages, 12 figures, accepted to ApJ

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Cited by in corpus (10)

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• Compositions of Planetary Debris around Dusty White Dwarfs
• The frequency of gaseous debris discs around white dwarfs
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