3C 66B
3C 66B | |
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观测资料(J2000 历元) | |
02h 23m 11.4112s[1] | |
+42° 59′ 31.385″[1] | |
红移 | 0.021258[1] |
距离 | 3亿 9,200 |
视星 | 15.0 (B) |
类型 | Sy1[1][3] FRI RG[2] |
2.4´X1.82´ | |
其他 | |
UGC 1841, LEDA 9067, 3C 66, 4C 42.07, PGC 9067, QSO B0220+427,[3] MAGIC J0223+430[4] | |
3C 66B (也称为3C 66)
3C 66B
![](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c0/HST-3C66B-jet-O5BQ06010.gif/220px-HST-3C66B-jet-O5BQ06010.gif)
距离
参考 资料
[编辑]- ^ 1.0 1.1 1.2 1.3 1.4 NASA/IPAC Extragalactic Database. Results for PGC 9067. [2006-10-26]. (
原始 内容 存 档于2019-09-18). - ^ 2.0 2.1 2.2 2.3 3C 66B. XJET: X-Ray Emission from Extragalactic Radio Jets. 2009-04-16 [2010-04-05]. (
原始 内容 存 档于2020-09-14). - ^ 3.0 3.1 3.2 SIMBAD. [2008-04-28]. (
原始 内容 存 档于2020-09-14). - ^ 4.0 4.1 Errando, Manel; Lindfors; Prandini; Tavecchio. A TeV source in the 3C 66A/B region. arXiv:0907.0994
.
- ^ Sudou, H.; Iguchi, S.; Murata, Y.; Taniguchi, Y. Orbital Motion in the Radio Galaxy 3C 66B: Evidence for a Supermassive Black Hole Binary. Science. 2003, 300 (5623): 1263–1265. PMID 12764190. doi:10.1126/science.1082817.
- ^ Jenet, F.; Lommen, A.; Larson, S. L.; Wen, L. Constraining the Properties of Supermassive Black Hole Systems Using Pulsar Timing: Application to 3C 66B. The Astrophysical Journal. 2004, 606 (2): 799–803. doi:10.1086/383020.
- ^ Perlin, Eric S.; Padgett; Georganopoulos; Sparks; Biretta; et al. Optical Polarimetry of the Jets of Nearby Radio Galaxies. I. The Data. The Astrophysical Journal. 2006, 651 (2): 735–748. Bibcode:2006ApJ...651..735P. doi:10.1086/506587.
外部 链接
[编辑]- www.jb.man.ac.uk/atlas/(页面
存 档备份,存 于互联网档案 馆) (J. P. Leahy) - 3C66B = B0220+427(页面
存 档备份,存 于互联网档案 馆) (Alan Bridle / 31 May 2006) - Wikisky image(页面
存 档备份,存 于互联网档案 馆) of PGC 9067