N76 vs NGC 248
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N76
N76 is a roughly 40-parsec H II shell in the Small Magellanic Cloud, notable for being ionized and shaped by the Wolf-Rayet binary AB 7.
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NGC 248
NGC 248 is an emission nebula and star-forming region in the Small Magellanic Cloud, a dwarf satellite galaxy of the Milky Way. It contains glowing hydrogen gas ionized by radiation from young, massive stars and is classified as an H II region. Scottish astronomer James Dunlop recorded the object in 1826, and it was later included in the New General Catalogue of Nebulae and Clusters of Stars.
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