N70 vs N44 (LMC)
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N70
N70, also known as Henize 70, is a large emission structure and superbubble in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It consists of gas shaped and energized by massive stars, stellar winds, and supernova activity, producing an expanding cavity that spans hundreds of light-years. Its Henize designation comes from Karl Henize's 1956 catalog of emission nebulae.
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N44 (LMC)
N44 is a large emission nebula and star-forming complex in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. Its gas is energized by nearby massive stars, and the complex contains dark dust lanes, stellar populations of different ages, and a prominent low-density cavity known as a superbubble. The cavity spans roughly 250 light-years, while the wider N44 complex extends for about 1,...
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