Search results
Results From The WOW.Com Content Network
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.
0 I 1656: Coma Cluster: Coma Berenices: 12 h 59 m 48.7 s +27° 58′ 50″ 2 II 1689: Virgo: 13 h 11 m 29.5 s: −01° 20′ 17″ 4 II-III One of the biggest and most massive galaxy clusters known; exhibits gravitational lensing. 1795: Boötes: 13 h 49 m 00.5 s +26° 35′ 07″ 2 I 1835: Virgo: 14 h 01 m 02.0 s +02° 51′ 32″ 0
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 ...
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 ...
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
Alter (open star clusters) (for example: Alter 1 at 0:31:56.9 / +63°09'47" in Cassiopeia) (Alter 1 = King 14 = Alter Cluster) Alves / Yun (open star clusters) AM — Arp-Madore catalogue of open and globular star clusters (Halton Arp / Barry F. Madore) (for example: Arp-Madore 1 in Horologium, Arp-Madore 2 in Puppis)
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]
NGC number Other names Object type Constellation Right ascension Declination Apparent magnitude; 6008: NGC 6008A Barred spiral galaxy: Serpens: 15 h 52 m 56.288 s +21° 06′ 01.819″ 12.9 6025: Open cluster: Triangulum Australe: 16 h 03 m 42 s: −60° 30′ 00″ 5.1 6027 (Part of Seyfert's Sextet) Interacting galaxy: Serpens: 15 h 59 m 12.7 ...