Best Sagitta
The Necklace Nebula is a ring-shaped planetary nebula located within the constellation Sagitta. It’s notable for its distinctive appearance formed by the interaction of a dying star with a companion star in a tight binary orbit. This orbital period of approximately 1.2 days significantly influences...
M1-67 is an emission nebula surrounding the Wolf-Rayet star WR 124 in the constellation Sagitta, roughly 20,000 light-years from Earth. The nebula consists of gas expelled by the massive, evolved star and shaped by its powerful stellar wind. Its irregular knots and clumps are moving outward, providi...
The Necklace Nebula is the common name for the planetary nebula IPHASXJ194359.5+170901, also catalogued as PN G054.2-03.4, in the constellation Sagitta. It contains a knotty, expanding ring of gas and fainter bipolar outflows extending roughly perpendicular to the ring. Observations show that the ce...
The Necklace Nebula (PN G054.2-03.4) is a planetary nebula located approximately 15,000 light-years from Earth in the northern constellation Sagitta. It was discovered in 2005 through the IPHAS H-alpha survey using the Isaac Newton Telescope. The nebula's distinctive ring of bright knots, resembling...
Sh2-82, commonly called the Little Cocoon Nebula, is a compact nebular complex in the constellation Sagitta. Cataloged in Stewart Sharpless's list of H II regions, it contains both reddish emission nebulosity from ionized hydrogen and bluish reflection nebulosity produced by scattered starlight. The...
M1-67 is an emission nebula surrounding WR 124, a runaway Wolf-Rayet star in the constellation Sagitta. The nebula consists of material expelled by the star and is notable for its irregular, knotty structure, which has been imaged in detail by the Hubble Space Telescope and the James Webb Space Tele...
Abell 63 is a planetary nebula in Sagitta, notable for the eclipsing binary central star UU Sagittae, linked to the nebula in 1976.
A Crab Nebula-analog pulsar wind nebula powered by a young energetic pulsar, and one of a small class of confirmed composite supernova remnants with a bright central synchrotron core.
A small, high-surface-brightness planetary nebula in Sagitta with a compact disk morphology, lying approximately 6,000 light-years from Earth and visible in modest telescopes.
