Fig. 17
(a) Soft X-ray emission mosaic in the 0.4–1.25 keV range (red) and MCELS Hα (cyan). Massive stars in the vicinity are marked with yellow crosses (O stars) and green circles (WR stars) (Bonanos et al. 2009). (b) Soft X-ray emission mosaic in the 0.4–1.25 keV range (red) and MCELS [S II]/Hα ratio ratio in green. Only ratio values above the threshold of 0.4 are shown. The vicinity of 30 Dor appears blank since we have very strong Hα emission here, thus yielding a very low ratio.
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