Fig. 1
Large-scale view of the L1495/B213 complex. The grey scale shows the Herschel-SPIRE 250 μm emission mapped by Palmeirim et al. (2013), and the red contours represent the N2H+(1–0) emission mapped by Hacar et al. (2013) with the FCRAO telescope. The black dashed lines show the limits of the FCRAO observations, and the blue solid lines enclose the regions newly mapped with the IRAM 30 m telescope.
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