NGC 1049
NGC 1049 is a globular cluster located in the Local Group galaxy of the Fornax Dwarf, visible in the constellation of Fornax. At a distance of 630,000 light years, it is visible in moderate sized telescopes, while the parent galaxy is nearly invisible. This globular cluster was discovered by John Herschel on October 19, 1835,[2] while the parent galaxy was discovered in 1938 by Harlow Shapley.[3]
NGC 1049 | |
---|---|
Observation data (J2000 epoch) | |
Class | V |
Constellation | Fornax |
Right ascension | 02h 39m 52.5s[1] |
Declination | −34° 16′ 08″[1] |
Distance | 630 ± ? kly (190 ± ? kpc) |
Apparent magnitude (V) | +12.9 |
Apparent dimensions (V) | 24″ |
Physical characteristics | |
Other designations | Hodge 3 |
References
- "SIMBAD Astronomical Database". Results for NGC 1049. Retrieved 2006-11-17.
- Seligman, Courtney. "NGC 1049 (= GCL 3 in the Fornax dwarf galaxy)". Celestial Atlas. Retrieved 7 December 2018.
- Shapley H (1938). "Two Stellar Systems of a New Kind". Nature. 142 (3598): 715–6. Bibcode:1938Natur.142..715S. doi:10.1038/142715b0.
External links
- Media related to NGC 1049 at Wikimedia Commons
- NGC 1049 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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