Delving into the depths of NGC 3783 with XRISM - IV. Mapping of the accretion flow with Fe Kα emission lines

Open Access

Fig. 8.

Best-fit inner radius as a function of spin (coloured lines). For each model, the best-fit inner radius is shown as a filled circle, together with the associated 1σ uncertainty from Table A.1. The prograde ISCO radius as a function of spin is shown as the dashed black line.

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