Fig. 28
Color composite image of the N 206 complex, constructed from the Herschel spire data (red: 500 μm), Hα (green: MCELS, Smith et al. 2005), and X-rays (blue: XMM-Newton 0.3−1 keV). CO intensity contours taken from the MAGMA survey are over-plotted to the image. The arrows suggest the possible leakage of hot gas from the X-ray superbubble.
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