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Fig. 14.
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Spectrum of an H II region along the VLT slit “3” at a projected distance of 25″ to the west of the pulsar (called filament F5 in Figs. 1 and 2). As in Fig. 11, we have also plotted spectra with expanded flux scales to highlight weaker lines. The spectrum have been dereddened using E(B − V) = 0.19 and RV = 3.1.
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