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Fig. 6

image

Best-fitting number Qion of ionizing photons at the illuminated face of the absorbing cloud of gas (divided by the quantity 4πc), vs. the best-fitting ionization parameter, U, for the three flux-interval spectra HS, MS and LS. Both the x and y-axis are in logarithmic scale. The straight line indicates the best-fitting linear relationship between log(Qion) and log (U), whose intercept provides an estimate for the quantity neR2 (see Sect. 4.2).

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