3C 66B
Appearance
3C66B | |
---|---|
![]() Hubble Legacy Archivevisible lightimage of 3C 66B | |
Observation data (J2000epoch) | |
Constellation | Andromeda |
Right ascension | 02h23m11.4112s[1] |
Declination | +42° 59′ 31.385″[1] |
Redshift | 0.021258[1] |
Distance | 300Mly(92Mpc)[2] |
Apparent magnitude(V) | 15.0 (B) |
Characteristics | |
Type | FRIRG[2] gamma-raysource[3] |
Apparent size(V) | 2.4´X1.82´ |
Other designations | |
3C66,4C42.07,QSOB0220+427[4],MAGIC J0223+430,2MASXJ02231141+4259313,UGC1841,LEDA9067,PGC9067[3] |
3C 66Bis anellipticalFanaroff and Riley class 1 radio galaxy[2]located in theconstellationAndromeda.With an estimatedredshiftof 0.021258,[1]the galaxy is about 300 millionlight-yearsaway.[2]
The orbital motion of 3C 66B showed supposed evidence for asupermassive black holebinary (SMBHB) with a period of 1.05 ± 0.03 years,[5]but this claim was later proven wrong (at 95% certainty).[6]
Messier 87(M87), about 55 million light-years away, is the largest giant elliptical galaxy near the Earth, and also contains anactive galactic nucleus.The smoothjetof 3C 66B rivals that of M87.[7]
3C 66B is an outlying member ofAbell 347which is part of thePerseus–Pisces Supercluster.[8]
![](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c0/HST-3C66B-jet-O5BQ06010.gif/250px-HST-3C66B-jet-O5BQ06010.gif)
References
[edit]- ^abcd"NASA/IPAC Extragalactic Database".Results for PGC 9067.RetrievedJune 25,2021.
- ^abcd"3C 66B".XJET: X-Ray Emission from Extragalactic Radio Jets. 2009-04-16.Retrieved2010-04-05.
- ^abErrando, Manel; Lindfors; Prandini; Tavecchio (2009). "A TeV source in the 3C 66A/B region".arXiv:0907.0994[astro-ph.HE].
- ^"UGC 1841 -- Seyfert 1 Galaxy".SIMBAD.RetrievedJune 25,2021.
- ^Sudou, H.; Iguchi, S.; Murata, Y.; Taniguchi, Y. (2003). "Orbital Motion in the Radio Galaxy 3C 66B: Evidence for a Supermassive Black Hole Binary".Science.300(5623): 1263–1265.arXiv:astro-ph/0306103.Bibcode:2003Sci...300.1263S.doi:10.1126/science.1082817.PMID12764190.S2CID36578161.
- ^Jenet, F.; Lommen, A.; Larson, S. L.; Wen, L. (2004). "Constraining the Properties of Supermassive Black Hole Systems Using Pulsar Timing: Application to 3C 66B".The Astrophysical Journal.606(2): 799–803.arXiv:astro-ph/0310276.Bibcode:2004ApJ...606..799J.doi:10.1086/383020.S2CID119457912.
- ^Perlin, Eric S.; Padgett; Georganopoulos; Sparks; Biretta; et al. (2006). "Optical Polarimetry of the Jets of Nearby Radio Galaxies. I. The Data".The Astrophysical Journal.651(2): 735–748.arXiv:astro-ph/0606119.Bibcode:2006ApJ...651..735P.doi:10.1086/506587.S2CID53073859.
- ^Fanti, C.; Fanti, R.; Feretti, L.; Ficarra, A.; Gioia, I. M.; Giovannini, G.; Gregorini, L.; Mantovani, F.; Marano, B. (1982-01-01). "Radio and optical observations of 9 nearby Abell clusters - A262, A347, A569, A576, A779, A1213, A1228, A2162, A2666".Astronomy and Astrophysics.105:200–218.Bibcode:1982A&A...105..200F.ISSN0004-6361.
External links
[edit]- www.jb.man.ac.uk/atlas/(J. P. Leahy)
- 3C66B = B0220+427(Alan Bridle / 31 May 2006)
- Wikiskyimageof PGC 9067