Sh2-311 vs NGC 2467
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Sh2-311
Sh2-311 is a large emission nebula and H II region in the constellation Puppis, also identified with NGC 2467. Its glowing gas is ionized by young, hot stars, and the surrounding complex contains active star formation, dark dust structures, and the young stellar groups Haffner 18 and Haffner 19. Infrared observations, including work with the Spitzer Space Telescope, have revealed embedded young st...
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NGC 2467
NGC 2467 is a vibrant emission nebula located within the Puppis constellation. It represents a complex star-forming region characterized by a dense cluster of young, hot stars. These massive stars intensely illuminate surrounding gas and dust, creating the nebula’s distinctive glow. Astronomers and researchers studying stellar evolution and active star formation find NGC 2467 particularly valuable...
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