NGC 5824
Appearance
NGC5824 | |
---|---|
Observation data (J2000epoch) | |
Constellation | Lupus |
Right ascension | 15h03m58.6s[1] |
Declination | –33° 04′ 07″[1] |
Distance | 104.4kly |
Apparent magnitude(V) | 9.09 |
Apparent dimensions(V) | 6.2' |
Physical characteristics | |
Metallicity | = –1.60[2]dex |
Estimated age | 12.80Gyr[2] |
Other designations | ESO 387-SC 001[1] |
NGC 5824is aglobular clusterin theconstellationLupus,almost on its western border withCentaurus.AstronomersJames Dunlop(1826),John Herschel(1831) andE.E. Barnard(1882) all claim to have independently discovered the cluster. It is condensed and may be observed with small telescopes, but larger apertures are required to resolve its stellar core.[3][4]
A stellar stream, known as the Triangulum stellar stream, is thought to have originated from NGC 5824. It is located quite far from NGC 5824 and is part of its leading tail. Meanwhile, its trailing tail has also been detected, spanning about 50 degrees through the sky.[5]
References
[edit]- ^abc"NASA/IPAC Extragalactic Database".Results for NGC 5824.Retrieved2007-04-06.
- ^abForbes, Duncan A.; Bridges, Terry (May 2010), "Accreted versus in situ Milky Way globular clusters",Monthly Notices of the Royal Astronomical Society,404(3): 1203–1214,arXiv:1001.4289,Bibcode:2010MNRAS.404.1203F,doi:10.1111/j.1365-2966.2010.16373.x,S2CID51825384.
- ^"NGC 5824 [Archive]".RetrievedJune 18,2011.
- ^"Deep-Sky Wonders".Sky & Telescope:226. August 1992.
- ^Yang, Yong; Zhao, Jing-Kun; Ishigaki, Miho N.; Chiba, Masashi; Yang, Cheng-Qun; Xue, Xiang-Xiang; Ye, Xian-Hao; Zhao, Gang (2022). "Existence of tidal tails for the globular cluster NGC 5824".Astronomy & Astrophysics.667:A37.arXiv:2208.05197.Bibcode:2022A&A...667A..37Y.doi:10.1051/0004-6361/202243976.S2CID251468198.
External links
[edit]- Media related toNGC 5824at Wikimedia Commons
- NGC 5824 onWikiSky:DSS2,SDSS,GALEX,IRAS,Hydrogen α,X-Ray,Astrophoto,Sky Map,Articles and images