N49 (LMC) vs N11
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N49 (LMC)
N49 is a supernova remnant in the Large Magellanic Cloud, a satellite galaxy of the Milky Way located in the southern sky. Its expanding shock structure is asymmetric and filamentary, and the remnant is associated with the soft gamma repeater SGR 0526-66, a source of recurring high-energy gamma-ray activity. N49 is studied through observations at X-ray and other wavelengths.
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N11
N11 is a large emission-nebula complex and H II region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is commonly described as the galaxy's second-largest star-forming region after the Tarantula Nebula and contains hot, young stars grouped in several OB associations. Stellar radiation and winds have ionized and reshaped the surrounding gas, producing shells, cavities, brigh...
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