3C 20 | |
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Observation data (J2000 epoch) | |
Constellation | Cassiopeia |
Right ascension | 00h 43m 09.18s[1][2] |
Declination | +52° 03′ 36.15″[1][2] |
Redshift | 0.174±0.001[3] |
Heliocentric radial velocity | 52,164±300 km/s[3] |
Galactocentric velocity | 52,352±300 km/s[3] |
Distance | 2,501 ± 175.5 Mly (766.7 ± 53.8 Mpc)h−1 0.6774 (Comoving)[3] 2.213 Gly (678.5 Mpc)h−1 0.6774 (Light-travel)[3] |
Apparent magnitude (V) | 19.0[3] |
Apparent magnitude (B) | 19.0[2] |
magnitude (J) | 16.368±0.112[4] |
magnitude (H) | 15.582±0.126[4] |
magnitude (K) | 14.756±0.115[4] |
Characteristics | |
Type | NLRG[3] |
Apparent size (V) | 76.8″ × 76.8″²[5] (radiogalaxy) |
Other designations | |
DA 22, 3C 20, LEDA 2817481 |
3C 20 is a radio galaxy[6] located in the constellation Cassiopeia. It features a prominent double hotspot in its eastern lobe. An unusually low fraction of the flux lies within the radio core, which is suggested to be caused by a combination of factors, including jet orientation, synchrotron self-absorption and aging, as well as interactions with surrounding gas and dust.[7]