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3C 215

Coordinates: Sky map 09h 06m 31.86s, +16° 46′ 11.9″
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3C 215
Observation data (Epoch J2000)
ConstellationCancer
Right ascension09h 06m 31.86s[1]
Declination+16° 46′ 11.9″[1]
Redshift0.411 551[1]
0.412 100[2]
Distance1,545 megaparsecs (5,040 Mly) h−1
0.73
[2]
TypeSy1, QSO, X, IR, G, blu[1]
QSO, FR II, Sy 1.5[2]
Apparent magnitude (V)18.27[1]
Other designations
DB 62, LEDA 2817602, 3C 215, 4C 16.26, QSO B0903+16
See also: Quasar, List of quasars

3C 215 is a Seyfert galaxy/Quasar located in the constellation Cancer.[1][2][3] This is a radio-loud quasar with a jet,[4] hosted in an elliptical galaxy and located inside a galaxy cluster. This object also shows signs of interaction with neighboring galaxy.[5]

3C 215 is also known to have a complex structure. Based on radio imaging, its inner region contains bright emission knots.[6]

References

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  1. ^ a b c d e f "Query : 3C 215". Simbad. Centre de Données astronomiques de Strasbourg. Retrieved 2 June 2015.
  2. ^ a b c d "NED results for object 3C 215". NASA/IPAC Extragalactic Database. Retrieved 2 June 2015.
  3. ^ Alan Bridle (6 November 1996). "3C215 = B0903+169". National Radio Astronomy Observatory (NRAO). Retrieved 2010-04-15.
  4. ^ Crawford, C. S.; Vanderriest, C. (2000-07-01). "Optical integral field spectroscopy of the extended line emission around six radio-loud quasars". Monthly Notices of the Royal Astronomical Society. 315 (3): 433–449. arXiv:astro-ph/9912306. doi:10.1046/j.1365-8711.2000.03290.x. ISSN 0035-8711.
  5. ^ Mei, A.; Tombesi, F. (2021-09-01). "XMM-Newton spectrum of the radio-loud quasar 3C 215: Slim accretion disk or SMBH binary". Astronomy & Astrophysics. 653: A100. arXiv:2107.14753. doi:10.1051/0004-6361/202140473. ISSN 0004-6361.
  6. ^ Lehnert, Matthew D.; Miley, George K.; Sparks, William B.; Baum, Stefi A.; Biretta, John; Golombek, Daniel; de Koff, Sigrid; Macchetto, Ferdinando D.; McCarthy, Patrick J. (August 1999). "HUBBLE SPACE TELESCOPE Snapshot Survey of 3CR Quasars: The Data". The Astrophysical Journal Supplement Series. 123 (2): 351–376. doi:10.1086/313239. ISSN 0067-0049.
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