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3C 9

From Wikipedia, the free encyclopedia
Quasar in the constellation of Pisces
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

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  1. ^ a b c d e f "3C 9". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019年11月20日.
  2. ^ a b c d "NASA/IPAC Extragalactic Database". Results for 3C 009. Retrieved 2010年04月20日.
  3. ^ "3C 9". XJET: X-Ray Emission from Extragalactic Radio Jets. 2009年03月26日. Retrieved 2010年04月06日.
  4. ^ a b Fabian, A. C.; Celotti, A.; Johnstone, R. M. (2003年01月01日). "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.
  5. ^ 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.
  6. ^ 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.
  7. ^ Time magazine, The Quasi-Quasars, Friday, June 18, 1965
[edit ]


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