| PKS 1148-001 | |
|---|---|
 PKS 1148-001 as observed by SDSS | |
| Observation data (J2000.0 epoch) | |
| Constellation | Virgo |
| Right ascension | 11h 50m 43.871s |
| Declination | -00d 23m 54.20s |
| Redshift | 1.979562 |
| Heliocentric radial velocity | 593,458 km/s |
| Distance | 10.221 Gly (light travel time distance) |
| Apparent magnitude (V) | 0.063 |
| Apparent magnitude (B) | 0.084 |
| Surface brightness | 17.1 |
| Characteristics | |
| Type | Opt var, RLQ |
| Other designations | |
| UM 458, 4C -00.47, PGC 37034, QUEST 042860, MRC 1148-001, MG1 J115044-0024, OM -480, TXS 1148-001, 1RXS J115044.2-002349, CoNFIG 113 | |
PKS 1148-001 also known as UM 458 and 4C -00.47, is a quasar located in the constellation of Virgo. Its redshift is 1.979, estimating the object to be located 10.2 billion light-years from Earth.[1]
Using interplanetary scintillations and very-long-baseline interferometry it was determined that the radio source associated with the quasar has an apparent size of 0.1 arcseconds.[2] An one-sided jet has been observed in the milliarcsecond scale. The most accepted theory for the creation of radio jets is the presence of a supermassive black hole which accretes material.[3]
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-06-12.
- ^ Venugopal, V. R.; Ananthakrishnan, S.; Swarup, G.; Pynzar, A. V.; Udaltsov, V. A. (1 August 1985). "Structure of PKS 1148-001". Monthly Notices of the Royal Astronomical Society. 215 (4): 685–689. doi:10.1093/mnras/215.4.685.
- ^ Kellermann, K. I.; Kovalev, Y. Y.; Lister, M. L.; Homan, D. C.; Kadler, M.; Cohen, M. H.; Ros, E.; Zensus, J. A.; Vermeulen, R. C.; Aller, M. F.; Aller, H. D. (10 October 2007). "Doppler boosting, superluminal motion, and the kinematics of AGN jets". Astrophysics and Space Science. 311 (1–3): 231–239. arXiv:0708.3219. Bibcode:2007Ap&SS.311..231K. doi:10.1007/s10509-007-9622-5.