Fig. 5.
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UV to optical spectral energy distribution of HU Aqr. Shown are the faint-phase data only, the accretion steam-corrected HST/FOS spectrum obtained 1996, and the OM data obtained simultaneously with the ULTRACAM u, g, r photometry. The model spectra for 13 500 K, 14 000 K, and 14 500 K scaled to the distance and radius of the white dwarf in HU Aqr are shown as blue lines.
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