Fig. 8.

XMM-Newton spectrum of the third observation of CI Cam with the best fit TBabs(TBabs(bbody+po)+Gaus+Gaus) model in red, with the intrinsic absorption (i.e. the second TBabs term) set to zero along with the best fit model to the outburst data from Ueda et al. (1998) in blue. The normalisation of the outburst model has been adjusted for easier comparison.
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