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3C 9
Quasar in the constellation of Pisces
Quasar in the constellation of Pisces
240,526 km/s QSO (light travel time){{cite web |access-date=2010-04-20 }} ~17 billion light-years (present comoving distance)
3C 9 is a lobe-dominated quasar{{cite web |access-date=2010-04-06}} located in the constellation Pisces. This quasar is classified as radio loud with a jet. It has X-ray emission located primary on two sides of its nucleus, based on Chandra observations.
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.
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.
References
References
- "3C 9".
- (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.
- (November 1982). "Extended radio jets in the high-redshift quasars 3C 9 and 280.1". Monthly Notices of the Royal Astronomical Society.
- (March 2021). "A Spatially Resolved Survey of Distant Quasar Host Galaxies. II. Photoionization and Kinematics of the ISM". The Astrophysical Journal.
- ''Time'' magazine, [https://web.archive.org/web/20080423044527/http://www.time.com/time/magazine/article/0,9171,898892,00.html The Quasi-Quasars], Friday, June 18, 1965
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