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• W2164383708 abstract "The 2006 outburst of GK Persei differed significantly at optical and ultraviolet (UV) wavelengths from typical outbursts of this object. We present multiwavelength (X-ray, UV and optical) Swift and AAVSO data, giving unprecedented broad-band coverage of the outburst, allowing us to follow the evolution of the longer-than-normal 2006 outburst across these wavelengths. In the optical and UV we see a triple-peaked morphology with maximum brightness ∼1.5 mag lower than in previous years. In contrast, the peak hard X-ray flux is the same as in previous outbursts. We resolve this dichotomy by demonstrating that the hard X-ray flux only accounts for a small fraction of the total energy liberated during accretion, and interpret the optical/UV outburst profile as arising from a series of heating and cooling waves traversing the disc, caused by its variable density profile." @default.
• W2164383708 created "2016-06-24" @default.
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• W2164383708 date "2009-11-01" @default.
• W2164383708 modified "2023-10-16" @default.
• W2164383708 title "The unusual 2006 dwarf nova outburst of GK Persei" @default.
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• W2164383708 doi "https://doi.org/10.1111/j.1365-2966.2009.15376.x" @default.
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