Emission nebula | |
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Planetary nebula | |
NGC 5979 by Hubble Space Telescope | |
Observation data: J2000 epoch | |
Right ascension | 15 47 41 |
Declination | −61° 13′ 05″ |
Apparent magnitude (V) | 12.10 |
Constellation | Triangulum Australe |
Physical characteristics | |
Radius | 0.51 ly |
Designations | NGC 5979, ESO 136-3, 2MASX J15474191-6113079 |
See also: Lists of nebulae |
NGC 5979 is a planetary nebula in the constellation Triangulum Australe. It was discovered by John Herschel on April 24, 1835. The central star of the planetary nebula is an O-type star with a spectral type of O(H)3-4.
Gallery
- NGC 5979 by Judy Schmidt
References
- ^ "NGC 5979". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 20 May 2019.
- Seligman, Courtney. "New General Catalog Objects: NGC 5950 - 5999". cseligman.com. Retrieved 23 May 2019.
- González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C.; López Varela, P. (2021). "Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity". Astronomy & Astrophysics. 656: A51. arXiv:2109.12114. Bibcode:2021A&A...656A..51G. doi:10.1051/0004-6361/202141916. S2CID 237940344.
External links
- NGC 5979 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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