In today's world, 3C 66A is an issue that has gained great relevance in society. As the years progress, the importance and impact of 3C 66A become more evident in different aspects of daily life. From its influence in the workplace to its impact on health and well-being, 3C 66A has become a constant topic of conversation in all types of spaces. In order to fully understand this phenomenon and its implications, it is crucial to analyze different perspectives and encourage constructive dialogue around 3C 66A. In this article, we will explore various aspects related to 3C 66A and its influence on today's society.
3C 66A | |
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![]() Hubble Legacy Archive WFPC2 image of 3C 66A (brightest object on the far right) | |
Observation data (Epoch J2000) | |
Constellation | Andromeda |
Right ascension | 02h 22m 39.612s[1] |
Declination | +43° 02′ 07.80″[1] |
Redshift | 0.444[1][2] |
Distance | 4.5 billion light-years (Light travel time)[2] 5.4 billion light-years (present)[2] |
Type | BLLAC[2] |
Apparent magnitude (V) | 15.5[1][2] |
Other designations | |
2E 558, 2EG J0220+4228, B3 0219+428A, QSO B0219+4248[1] | |
See also: Quasar, List of quasars |
3C 66A is a blazar[1][2] located in the constellation Andromeda.
The "distance" of a far away galaxy depends on the distance measurement used. With a redshift of 0.444,[1][2] light from this active galaxy is estimated to have taken around 4.5 billion years to reach Earth.[2] But as a result of the expansion of the Universe, the present (co-moving) distance to this galaxy is about 5.4 billion light-years (1647 Mpc).[2] Even at this great distance this blazar has an apparent magnitude of about 15.5.[1] Although 0.444 is used as the common redshift value, 0.3347 is a new strict lower limit "inferred through observing the far-UV absorption by the low-z IGM."[3]
3C 66A underwent an optical outburst in 2007 August, as monitored by the Tuorla blazar monitoring program.[4] The event was monitored by the Whole Earth Blazar Telescope project.