| NGC 6045 | |
|---|---|
 Sloan Digital Sky Survey image of NGC 6045. The small, nearby galaxy at left portion of the image is PGC 84720. | |
| Observation data (J2000 epoch) | |
| Constellation | Hercules |
| Right ascension | 16h 05m 07.9s[1] |
| Declination | 17° 45′ 28″[1] |
| Redshift | 0.033310[1] |
| Heliocentric radial velocity | 9986 km/s[1] |
| Distance | 137 Mpc (447 Mly)[1] |
| Group or cluster | Hercules Cluster |
| Apparent magnitude (V) | 14.9[1] |
| Characteristics | |
| Type | SB(s)c[1] |
| Size | ~183,300 ly (56.20 kpc)[1] (estimated)[1] |
| Apparent size (V) | 1.17 x 0.28[1] |
| Notable features | Warped disk |
| Other designations | |
| PGC 057031, UGC 10177, Arp 71, MCG +03-41-088[1] | |
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NGC 6045 is a barred spiral galaxy located about 450 million light-years away[2] in the constellation Hercules.[3] NGC 6045 was discovered by astronomer Lewis Swift on June 27, 1886[4] and is a member of the Hercules Cluster.[5][4] It is also a LINER galaxy.[6]
- ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 6045. Retrieved 2018-02-01.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-02-02.
- ^ "Revised NGC Data for NGC 6045". spider.seds.org. Retrieved 2018-02-02.
- ^ a b "New General Catalog Objects: NGC 6000 - 6049". cseligman.com. Retrieved 2018-01-25.
- ^ Huang, Zhenping; Sarazin, Craig L. (April 1996). "A High-Resolution ROSAT X-Ray Study of the Hercules Cluster". The Astrophysical Journal. 461: 622. Bibcode:1996ApJ...461..622H. doi:10.1086/177090. ISSN 0004-637X.
- ^ "NGC 6045". Retrieved 2018-08-17.