Astronomy:4C +37.11
| 4C +37.11 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Perseus |
| Right ascension | 04h 05m 49.2s[1] |
| Declination | +38° 03′ 32″[1] |
| Redshift | 16,500 ± 300 km/s[1] |
| Distance | 750 Mly (230 Mpc) [2] |
| Apparent magnitude (V) | 17.2[1] |
| Characteristics | |
| Type | Sy[1] |
| Size | ~450,400 ly (138.10 kpc) (estimated)[1] |
| Other designations | |
| GLXY J0405+380, B2 0402+37, 2MASX J04054928+3803320, RX J0405.8+3803, PGC 2820486 | |
4C +37.11 or Galaxy 0402+379 is a radio galaxy and elliptical galaxy featuring binary supermassive black holes with the least separation of any directly observed binaries, as of 2006. The separation between the two is 24 light-years or 7.3 parsecs, with an orbital period of 30,000 years. The two supermassive black holes, about 750 million light years from earth (230 million parsecs from earth), have a current estimated combined mass of about 28 ± 8 billion M☉.[3]
Other supermassive binary black hole candidates suggest the smaller separation distances expected as they eventually merge, but have not been confirmed. For example, quasar OJ 287 is inferred to have a binary supermassive black hole pair with an orbital period of 12 years, and thus be much closer together. However these have not been directly measured and additional observation, possibly over extended time periods, is needed.
The eventual collision of the pair, which should stay apart for at least a few million more years, would result in strong gravitational waves.[4]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "NASA/IPAC Extragalactic Database". Results for 0402+379. http://nedwww.ipac.caltech.edu/.
- ↑ "Scientists Find Closest Pair of Supermassive Black Holes". PhysOrg.com. http://www.physorg.com/news65714406.html.
- ↑ Surti, Tirth; Romani, Roger W.; Scharwächter, Julia; Peck, Alison; Taylor, Greg B. (5 January 2024). "The Central Kinematics and Black Hole Mass of 4C+37.11". The Astrophysical Journal 960 (2): 6. doi:10.3847/1538-4357/ad14fa. ISSN 1538-4357. Bibcode: 2024ApJ...960..110S.
- ↑ Klesman, Alison (29 June 2017). "Astronomers spot a pair of orbiting supermassive black holes". Astronomy Magazine. http://www.astronomy.com/news/2017/06/orbiting-smbhs.
- VLBA Reveals Closest Pair of Supermassive Black Holes (UNM Today) 2 May 2006
- A Compact Supermassive Black-Hole Binary System (Los Alamos National Laborator - LANL)
External links
- Black Hole Pair Sets Proximity Record (SPACE.com) 1 May 2006 02:04 pm ET
- Two black holes come oh-so-close (MSNBC) 5:23 p.m. ET 1 May 2006
- Colossal black holes seen in closest clinch yet (New Scientist) 16:02 21 April 2006
- A Supermassive Black Hole Pairing (Centauri Dreams)
- Scientists Find Closest Pair of Supermassive Black Holes (PhysOrg.com) 1 May 2006
- VLBA Reveals Closest Pair of Supermassive Black Holes (SpaceRef.com) Monday, 1 May 2006
- Closest-spaced giant black hole pair found (SpaceFlight Now) 1 May 2006
Coordinates: 
04h 05m 49.2s, 38° 03′ 32″
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