In this article we are going to address the issue of 3C 223, which has gained great relevance in recent years. 3C 223 is a topic that has aroused the interest of experts and the general public, due to its impact on various areas of society. Throughout this article we will explore different aspects of 3C 223, from its origins to its current implications. Likewise, we will analyze the different perspectives and approaches that have been developed around this topic, in order to offer a broad and complete vision of 3C 223. Without a doubt, this is an exciting topic that promises to generate an enriching debate and shed light on fundamental issues for understanding current reality.
3C 223 | |
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![]() The galaxy 3C 223. | |
Observation data (Epoch J2000) | |
Constellation | Leo Minor |
Right ascension | 09h 39m 52.761s[1] |
Declination | +35° 53′ 58.91″[1] |
Redshift | 0.136730[2] |
Distance | 549 Mpc (1.79 billion ly) h−1 0.73[2] |
Type | Sy2, Rad, AGN, G, QSO, X, gam[1] G[2] |
Apparent magnitude (V) | 18.60[1] |
Other designations | |
DA 269, LEDA 27575, 4C 36.16, QSO B0936+361 | |
See also: Quasar, List of quasars |
3C 223 is a Seyfert galaxy[1] located in the constellation of Leo Minor. It hosts a Type 2 quasar nucleus, found to be radio-loud with a rare, Compton-thick active galactic nucleus.[3][4]
3C 223 is also a radio galaxy.[5] With a projected size of ≥1 megaparsecs, it is classified a giant radio source according to researchers who presented Very Large Array images. Based on spectral study results, the source of 3C 223 is found to be younger.[6]