Sh2-297 vs Sh2-101
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Sh2-297
Sh2-297 is an emission nebula and H II region in the constellation Canis Major, catalogued by Stewart Sharpless in his 1959 survey of Galactic ionized-hydrogen regions. It forms part of the broader CMa OB1 star-forming complex and contains gas illuminated by nearby hot stars. Astronomers study the region for its embedded young stellar objects, molecular material, and evidence of continuing star fo...
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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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