Astronomy:Abell 569
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Short description: Galaxy cluster in the constellation Lynx
| Abell 569 | |
|---|---|
| File:Abell 569 by DESI Legacy Surveys.png Abell 569 seen by DESI Legacy Surveys DR11 | |
| 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]
Abell 569 is a galaxy cluster located in the Supercluster 32 (SCL 32) along with 3 other members namely, Abell 568, Abell 581 and Abell 599 using estimated redshifts.[3]
See also
Gallery
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Abell 569 seen by DESI Legacy Surveys
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Abell 569
References
- ↑ 1.0 1.1 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, doi:10.1046/j.1365-8711.2001.04786.x, Bibcode: 2001MNRAS.327..265H.
- ↑ 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.
- ↑ Einasto, M.; Einasto, J.; Tago, E.; Andernach, H.; Dalton, G. B.; Müller, V. (2001). "Optical and X-Ray Clusters as Tracers of the Supercluster-Void Network. III. Distribution of Abell and APM Clusters". The Astronomical Journal 122 (5): 2222–2242. doi:10.1086/323141. Bibcode: 2001AJ....122.2222E.
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