N49 vs N132D
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N49
N49 is a supernova remnant in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is observed at optical, radio, infrared, and X-ray wavelengths, where its expanding shock interacts with uneven surrounding interstellar material and produces a complex filamentary structure. N49 is also associated with SGR 0526-66, the soft gamma repeater responsible for the intense gamma-ray event d...
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N132D
N132D is an oxygen-rich supernova remnant in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is a strong X-ray source whose expanding debris contains enhanced oxygen and other elements produced inside the massive progenitor star before its explosion. Astronomers study N132D across X-ray, optical, and infrared wavelengths to examine supernova ejecta, shock interaction with surro...
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