Most white dwarfs with detectable dust discs show infrared variability

Abstract

Archival data from the WISE satellite reveals infrared flux variations of tens of per cent around numerous dusty white dwarfs. Data spanning more than seven years reveal more than half of known systems are varying in the 3.4 micron band, while the 4.6 micron data are challenging to interpret due to lower signal-to-noise. The sparsely-sampled data limit interpretation, but the heterogeneous light curves suggest each source may be idiosyncratic, where there maybe competing processes operating on different time-scales. Collisions are likely driving the observed decays in flux, and this finding suggests that dust production is operating more often than indicated by previous observations. The observed variation is at odds with the canonical flat disc model in isolation, and underscores the need for infrared monitoring of these evolved planetary systems to inform the next generation of theoretical models.

5 pages; accepted to MNRAS Letters

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• Shallow Ultraviolet Transits of WD 1145+017
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• The grain size survival threshold in one-planet post-main-sequence exoplanetary systems
• Asteroid belt survival through stellar evolution: dependence on the stellar mass