Fig. 9
Left panels: rotated Chandra soft X-ray images for 3C 403 (top) and 3C 445 (bottom) with the superposed 2″ wide slit used to obtain the spectra at the TNG shown in the right panels. The three emission lines are Hβ and the [0 III]λλ4959, 5007 doublet. Substantial line emission is produced along the direction of the soft X-ray emission. The sizes of the two emitting regions (in line and X-rays) are similar.
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