NGC 1128
| NGC 1128 | |
|---|---|
 Binary black hole system 3C 75 contained in the dumbbell shaped galaxy NGC 1128 | |
| Observation data (J2000 epoch) | |
| Right ascension | 2h 57m 41.6s[1] |
| Declination | +6° 01′ 29″[1] |
| Redshift | 6940 ± 20 km/s[1] |
| Distance | 300 Mly[2] |
| Apparent magnitude (V) | 13.8[1] |
| Characteristics | |
| Type | E0[1] |
| Apparent size (V) | 0'.9 × 0'.4[1] |
| Notable features | Dumbbell-shaped galaxy |
| Other designations | |
| PGC 11188[1] | |
NGC 1128 is a "dumbbell galaxy" in the Abell 400 galaxy cluster. It is the center of the 3C75 radio source and contains two orbiting supermassive black holes that may be merging. Computer simulations indicate that these two black holes will gradually spiral in toward each other until they merge. Lewis Swift is credited with the discovery of NGC 1128 in 1886.[3]
References
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for. Retrieved 2006-10-26.
- ^ http://antwrp.gsfc.nasa.gov/apod/astropix.html
- ^ Seligman, Courtney. "Celestial Atlas: NGC Objects: NGC 1100 - 1149". cseligman.com. Archived from the original on 25 July 2015. Retrieved 25 July 2015.
External links
- Black Holes Dance With Incredible Violence (SpaceDaily) Apr 12, 2006
- 3C 75 in Abell 400: Black Holes Determined to be Bound (Chandra AXAF)
- More Images of 3C 75 in Abell 400 (Chandra AXAF)
- NGC 1128 (jpeg, Chandra AXAF)
- NGC 1128 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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