Image obtained from the combination of hydrogen, sulfur and oxygen bandpasses (Magellanic Clouds Emission-Line Survey MCELS, C. Aguilera, C. Smith and S. Points/NOAO/AURA/NSF). Contours correspond to the CO(2–1) line emission. We indicate the position of the OB associations in N11, LH9 in the central cavity of N11, LH10 in the nebula N11B, LH13 in N11C and LH14 in N11E.
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