Abell 569

Abell 569
Observation data (Epoch J2000)
Constellation(s)	Lynx
Right ascension	07h 09m 10.4s
Declination	+48° 37′ 10″
Bautz–Morgan classification	II
Velocity dispersion	500 [1]
Redshift	0.019417 [1]
Other designations
A 569

Abell 569 is a galaxy cluster in the northern constellation of Lynx. It is organized into two primary condensations that are separated by about 1.5 Mpc, and is probably a member of the Perseus Supercluster. The brightest galaxy in the cluster is NGC 2329, a giant elliptical galaxy of type D that is associated with a radio and X-ray source. ^[2]

References

1. Hudson, Michael J.; et al. (October 2001), "Streaming motions of galaxy clusters within 12 000 km s-1 - III. A standardized catalogue of Fundamental Plane data", Monthly Notices of the Royal Astronomical Society, 327 (1): 265–295, Bibcode:2001MNRAS.327..265H, doi: 10.1046/j.1365-8711.2001.04786.x , hdl: 10533/172647 .
2. Feretti, L.; et al. (June 1985), "The wide angle tailed radio source NGC 2329 in the cluster A 569", Astronomy and Astrophysics, 147 (2): 321–327, Bibcode:1985A&A...147..321F.