Fig. 6
Top: cumulative absorption column density (dot-dashed line) together with the 12CO and HI contributions as a function of the radial velocity integrated on a 0.1° box region centered on the pulsar. Bottom: corresponding 12CO and HI spectra at the position of the pulsar. The Vela molecular ridge, centered at VLSR ~ 5 km s-1, is the main 12CO structure along the pulsar’s line of sight.
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