NGC 2440 vs NGC 2452
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NGC 2440
NGC 2440 is a planetary nebula located within the constellation Puppis. It’s recognized for its intricate, multi-lobed structure formed by the outflow of gas from a dying star. At its center lies a white dwarf emitting intense heat, reaching temperatures approaching 200,000 Kelvin. Astronomers and researchers studying stellar evolution and the processes surrounding planetary nebula formation find...
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NGC 2452
NGC 2452 is a planetary nebula in the southern constellation Puppis. John Herschel discovered it in 1847, and catalogues place it about 15,000 light-years from Earth, separate from the nearby open cluster NGC 2453 even though the two objects appear close together in the sky. Its central star has the hydrogen-deficient [WO1] spectral classification, marking it as a hot stellar remnant at the centre...
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