UV spectroscopy of the 44 nearest white dwarfs reveals a 2–6% temperature discrepancy between UV and optical model fits, six UV-only metal detections, and a 30% planetary debris accretion rate.
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2020, series =
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White dwarfs within 13 pc: Insights from ultraviolet spectroscopy
UV spectroscopy of the 44 nearest white dwarfs reveals a 2–6% temperature discrepancy between UV and optical model fits, six UV-only metal detections, and a 30% planetary debris accretion rate.