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The second most massive galaxy cluster next to El Gordo is RCS2 J2327, a galaxy cluster with the mass of 2 quadrillion suns. Also has a systematic designation of ACT-CL J0102-4915. [6] [7] [8] Musket Ball Cluster: Named in comparison to the Bullet Cluster, as this one is older and slower galaxy cluster merger than the Bullet Cluster.
Pages in category "Galaxy clusters" The following 138 pages are in this category, out of 138 total. ... 0–9. 2XMM J083026+524133; A. Abell 68; Abell 222; Abell 223 ...
Globular Cluster: 17.3 Centaurus: 3.7 C81 NGC 6352 Globular Cluster: 18.6 Ara: 8.2 C82 NGC 6193 Open Cluster: 4.3 Ara: 5.2 C83 NGC 4945 Barred Spiral Galaxy: 17,000 Centaurus: 9 C84 NGC 5286 Globular Cluster: 36 Centaurus: 7.6 C85 IC 2391: Omicron Velorum Cluster: Open Cluster: 0.5 Vela: 2.5 C86 NGC 6397 Globular Cluster: 7.5 Ara: 5.7 C87 NGC ...
Comprises such a huge amount of mass that the galaxy cluster noticeably curves spacetime around it, making it into a gravitational lens. Smaller galaxies behind the cluster appear distorted into long, warped arcs around the cluster’s edges. [7] 3266: Horologium Supercluster: Reticulum: 04 h 31 m 11.9 s: −61° 24′ 23″ 2 I-II 3341: 05 h ...
These four near-equals at the core of galaxy cluster CL 0958+4702 are in the process of merging. [149] Galaxy protocluster LBG-2377: z=3.03 This was announced as the most distant galaxy merger ever discovered. It is expected that this proto-cluster of galaxies will merge to form a brightest cluster galaxy, and become the core of a larger galaxy ...
MACS J0152.5-2852 is a massive galaxy cluster. Almost every pixel seen in the image is a galaxy, each containing billions of stars. [1]Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. [2]
The following are lists of clusters: List of galaxy groups and clusters; List of open clusters ... Text is available under the Creative Commons Attribution-ShareAlike ...
Abell divided the clusters into six "richness groups", depending on the number of galaxies in a given cluster that lie within the magnitude range m 3 to m 3 +2 (the average number of galaxies per cluster for the entire catalog was 64): Group 0: 30–49 galaxies; Group 1: 50–79 galaxies; Group 2: 80–129 galaxies; Group 3: 130–199 galaxies