MRC 2011-298 | |
---|---|
Observation data (J2000.0 epoch) | |
Constellation | Sagittarius |
Right ascension | 20h 14m 18.86s |
Declination | -29d 42m 36.02s |
Redshift | 0.136620 |
Heliocentric radial velocity | 40,958 km/s |
Distance | 2.115 Gly (648.5 Mpc) |
Group or cluster | Abell 3670 |
Apparent magnitude (V) | 0.229 |
Apparent magnitude (B) | 0.303 |
Characteristics | |
Type | E |
Notable features | Radio galaxy |
Other designations | |
PMN J2014-2942, PGC 726073, NVSS J201418-294234, TXS 2011-298, 2MASX J20141866-2942364 |
MRC 2011-298 is an elliptical galaxy with an active galactic nucleus, located in the constellation of Sagittarius. It is located 2.1 billion light-years away from Earth. MRC 2011-298 is the brightest cluster galaxy in the galaxy cluster, Abell 3670[1][2] and classfied as a dumbbell galaxy,[3] an optical system with two galactic nuclei separated by 7″, corresponding to ≃17 kpc according to the adopted cosmology, with similar magnitude and a common stellar halo.[4] The galaxy is known to have an ellipticity of ε = 0.28 and a position angle of PA = 24° that is measured from north to east.[5]