Fig. 2
RGS1+2 fluxed spectrum of V2491 Cyg fitted in the range 7–14.4 Å using the plasma emission model Cie and the cold Hot-ISM absorption model. A blackbody model of emission was also used as an additive model for the second-observation spectrum. The left- and right-hand panels show the fit to the fluxed spectrum of region 3 and second-observation data, respectively.
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