This is a composite image of the brightest supernova remnant in optical light in the Large Magellanic Cloud. The Chandra X-ray image (blue) shows million-degree gas in the center. Much cooler gas at the outer parts of the remnant is seen in.
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in the LMC - Southern part of the spectacular H II region in the Large Magellanic Cloud. The green color indicates areas that are particularly hot. The field measures x square arcminutes. North is up and East is left.