3C 9
| 3C 9 | |
|---|---|
| Observation data (Epoch J2000) | |
| Constellation | Pisces |
| Right ascension | 00h 20m 25.22s |
| Declination | +15° 40′ 54.7″ |
| Redshift | 2.0194[1] 240,526 km/s[1] |
| Distance | 10 billion light-years (light travel time)[2] ~17 billion light-years (present comoving distance)[2] |
| Type | FR II RG[2] QSO[1][2] |
| Apparent magnitude (V) | 17.62[1] |
| Other designations | |
| 2C 26, LEDA 2817473[1] | |
| See also: Quasar, List of quasars | |
3C 9 is a lobe-dominated quasar[1][3] located in the constellation Pisces. This quasar is classified as radio loud with a jet.[4][5] It has X-ray emission located primary on two sides of its nucleus, based on Chandra observations.[4]
The host of 3C 9 is described as a ring-like galaxy undergoing a merger. The two nuclei of the merging galaxies are estimated to be 9 kiloparsecs apart.[6]
In 1965, it was the most distant object discovered at the time of discovery. This was the first object found with a redshift in excess of 2.[7]
References
[edit]- 1 2 3 4 5 6 "3C 9". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-11-20.
- 1 2 3 4 "NASA/IPAC Extragalactic Database". Results for 3C 009. Retrieved 2010-04-20.
- ↑ "3C 9". XJET: X-Ray Emission from Extragalactic Radio Jets. 2009-03-26. Retrieved 2010-04-06.
- 1 2 Fabian, A. C.; Celotti, A.; Johnstone, R. M. (2003-01-01). "Chandra reveals X-rays along the radio axis in the quasar 3C 9 at z= 2.012". Monthly Notices of the Royal Astronomical Society. 338 (1): L7–L11. arXiv:astro-ph/0204488. doi:10.1046/j.1365-8711.2003.06111.x. ISSN 0035-8711.
- ↑ Swarup, G.; Sinha, R. P.; Saikia, D. J. (November 1982). "Extended radio jets in the high-redshift quasars 3C 9 and 280.1". Monthly Notices of the Royal Astronomical Society. 201 (2): 393–400. doi:10.1093/mnras/201.2.393. hdl:1887/6417. ISSN 0035-8711.
- ↑ Vayner, Andrey; Wright, Shelley A.; Murray, Norman; Armus, Lee; Boehle, Anna; Cosens, Maren; Larkin, James E.; Mieda, Etsuko; Walth, Gregory (March 2021). "A Spatially Resolved Survey of Distant Quasar Host Galaxies. II. Photoionization and Kinematics of the ISM". The Astrophysical Journal. 910 (1): 44. arXiv:2101.08291. doi:10.3847/1538-4357/abddc1. ISSN 0004-637X.
- ↑ Time magazine, The Quasi-Quasars, Friday, June 18, 1965
