Sh2-311 vs Sh2-101
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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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Sh2-101
Sh2-101 is an emission nebula within the Cygnus constellation. It’s a Sharpless H II region, specifically known as the Tulip Nebula due to its distinctive flower-like shape. This star-forming area is notable for its proximity to the black hole binary system Cygnus X-1. Astronomers and researchers studying stellar nurseries and active galactic nuclei find it particularly relevant.
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