Fig. 3

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Spatial distribution of multiwavelength emissions within the N11 analysis region highlighted by white squares in Figs. 2 and 1. (a) Optical three-color image with Hα (red), [SII] (green), and [OIII] (blue) (Smith et al. 2005). (b) Soft X-ray emission (0.2–0.5 keV) toward the N11 source region. White lines show the four extraction regions of the spectra. Black crosses and asterisks are O-type stars and WR stars (Bonanos et al. 2009), respectively. (c) Spatial distribution of the total hydrogen column density NH. The contour levels are 1.5 × 1021, 3.0 × 1021, 4.5 × 1021, and 6.0 × 1021 cm−2. The white box indicates the region shown in Fig. 7. (d) The total hydrogen column density map by contours superposed on soft X-ray emission (0.2–0.5 keV).
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