3C 303
(Redirected from QSO B1441+5214)
| 3C 303 | |
|---|---|
 | |
| Observation data (Epoch J2000) | |
| Constellation | Boötes |
| Right ascension | 14h 43m 02.76070s[1] |
| Declination | +52° 01′ 37.2982″[1] |
| Redshift | 0.141186[2] |
| Distance | 564 megaparsecs (1.84×109 ly) h−1 0.73[2] |
| Type | Sy1, Rad, AGN, IR, X, AG?, QSO, G[1] G, FR II, Sy 1.5[2] |
| Apparent magnitude (V) | 18.29[1] |
| Other designations | |
| DA 369, 3C 303, QSO B1441+5214 | |
| See also: Quasar, List of quasars | |
3C 303 is a Seyfert galaxy[1][2] with a quasar-like appearance located in the constellation Boötes.
3C 303 is also a radio galaxy[3] It also contains an extragalactic radio source.[4] A clear defined jet is also seen, showing a polarization variation trend. With a diffuse patch of optical emission located at the intersection of the jet where a radio lobe is connected, the jet is confirmed to target a region of interstellar medium.[5]
References
[edit]- ^ a b c d e "Query : 3C 303". Simbad. Centre de Données astronomiques de Strasbourg. Retrieved 2 June 2015.
- ^ a b c d "NED results for object 3C 303". NASA/IPAC Extragalactic Database. Retrieved 2 June 2015.
- ^ Kataoka, J.; Edwards, P.; Georganopoulos, M.; Takahara, F.; Wagner, S. (2003-02-01). "Chandra detection of hotspot and knots of 3C 303". Astronomy & Astrophysics. 399 (1): 91–97. doi:10.1051/0004-6361:20021772. ISSN 0004-6361.
- ^ Lonsdale, C. J.; Hartley-Davies, R.; Morison, I. (January 1983). "The radio structure of 3C 303 at 408 MHz". Monthly Notices of the Royal Astronomical Society. 202 (1): 1P–5P. doi:10.1093/mnras/202.1.1p. ISSN 0035-8711.
- ^ Kronberg, P. P. (1986-04-01). "3C 303: a "laboratory" extragalactic jet source". Canadian Journal of Physics. 64 (4): 449–451. Bibcode:1986CaJPh..64..449K. doi:10.1139/p86-081. ISSN 0008-4204.
External links
[edit]- www.jb.man.ac.uk/atlas/ (J. P. Leahy)
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