Sh2-91 vs Sh2-225
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Sh2-91
Sh2-91 is a very faint emission nebula located in the northern constellation of Cygnus. It is classified as part of the Sharpless catalog and is specifically identified as the long southern filament of the supernova remnant designated G65.2+5.7. Because of its extremely low surface brightness, it is a challenging target for visual observation and requires specialized astrophotography equipment to...
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Sh2-225
Sh2-225 is an emission nebula and H II region in the constellation Auriga. It lies in the Milky Way's Perseus Arm and is catalogued in the Sharpless list of H II regions. The region is associated with ionized hydrogen and an embedded infrared source, making it a subject of observations of massive-star formation; one proposed ionizing star is the O-type star LSV+4046. Because it is faint and compac...
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