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Fig. 8.
Faint-phase EPIC-MOS (main panel) and -pn (inset) spectra of AM Herculis obtained 2005 with best-fit model spectra overplotted. Observed data were binned with a minimum of 25 counts per spectral bin. Two model components are shown, the soft blackbody and the sum of all others originating from the accretion plasma
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