PKS J1158+2621
From Wikipedia, the free encyclopedia
| PKS J1158+2621 | |
|---|---|
SDSS image of PKS J1158+2621. | |
| Observation data (J2000.0 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 58m 20.14s[1] |
| Declination | +26° 21′ 12.00″[1] |
| Redshift | 0.112023[1] |
| Heliocentric radial velocity | 33,584 km/s[1] |
| Distance | 1.507 Gly |
| Apparent magnitude (V) | 18.5 |
| Characteristics | |
| Type | E[1] |
| Size | ~271,000 ly (83.08 kpc) (estimated)[1] |
| Other designations | |
| 4C 26.35, CLASS J1158+2621, LEDA 97402, 2MASX J11582015+2621120, 4C 26.35A, 7C 1155+2637, ABELL 1425:[OWG93][1] | |
PKS J1158+2621 is a low-ionization nuclear emission line region (LINER) galaxy located in the constellation of Leo. The redshift of the galaxy is (z) 0.112[1] and it was first discovered as an astronomical radio source by E.T. Olsen at Owens Valley Radio Observatory in California in August 1967, where it was given the designation as 4C 26.35 or 4C 26.35A.[2][3] It is classified as a radio galaxy[4] and is one of the brightest known cluster galaxies in Abell 1425 although being nondominant.[3][5]