Hidden supernova remnants in the Large Magellanic Cloud H II complex N44
We have obtained ROSAT PSPC observations of N44, one of the largest H II complexes in the Large Magellanic Cloud. The X-ray emission mostly fails within the ionized shell structures in N44. We find that one faint shell is a classical supernova remnant overlooked by previous surveys. If we model the two largest shells as pressure-driven superbubbles
Kennicutt, Robert C., Jr. et al.
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1993