2029 |
|
|
Virgo |
15h 10m 56.0s |
+05° 44′ 41″ |
2 |
I |
Near the Serpens–Virgo border. |
2052 |
|
|
|
15h 16m 45.5s |
+07° 00′ 01″ |
0 |
I-II |
|
2061 |
|
Corona Borealis Supercluster |
Corona Borealis |
15h 21m 15.3s |
+30° 39′ 17″ |
1 |
III |
|
2063 |
|
Hercules Superclusters |
|
15h 23m 05.3s |
+08° 36′ 33″ |
|
|
|
2065 |
Corona Borealis Cluster |
Corona Borealis Supercluster |
Corona Borealis |
15h 22m 42.6s |
+27° 43′ 21″ |
2 |
III |
|
2067 |
|
Corona Borealis Supercluster |
Corona Borealis |
15h 23m 14s |
+30° 54′ 23″ |
1 |
III |
|
2079 |
|
Corona Borealis Supercluster |
Corona Borealis |
15h 28m 04.7s |
+28° 52′ 40″ |
|
|
|
2089 |
|
Corona Borealis Supercluster |
Corona Borealis |
15h 32m 41.3s |
+28° 00′ 56″ |
|
|
|
2092 |
|
Corona Borealis Supercluster |
Corona Borealis |
15h 33m 17.0s |
+31° 08′ 55″ |
|
|
|
2107 |
|
Hercules Superclusters |
|
15h 39m 39.0s |
+21° 46′ 58″ |
|
|
|
2124 |
|
|
Corona Borealis |
15h 44m 59s |
+36° 04′ |
1 |
I |
|
2142 |
|
|
Corona Borealis |
15h 58m 16.1s |
+27° 13′ 29″ |
2 |
II |
A merger of two huge galaxy clusters. |
2147 |
|
Hercules Superclusters |
Serpens |
16h 02m 17.2s |
+15° 53′ 43″ |
1 |
III |
|
2151 |
Hercules Cluster |
Hercules Superclusters |
Hercules |
16h 05m 15.0s |
+17° 44′ 55″ |
2 |
III |
Major component of the Hercules Superclusters. |
2152 |
|
Hercules Superclusters |
|
16h 05m 22.4s |
+16° 26′ 55″ |
1 |
III |
The smaller part of the Hercules supercluster, Lx ≤ 3 x 1044 ergs/s.[5] |
2162 |
|
Hercules Superclusters |
Corona Borealis |
16h 12m 30.0s |
+29° 32′ 23″ |
|
|
|
2163 |
|
|
Ophiuchus |
16h 15m 34.1s |
−06° 07′ 26″ |
2 |
|
|
2199 |
|
Hercules Superclusters |
Hercules |
16h 28m 38.5s |
+39° 33′ 06″ |
2 |
I |
|
2200 |
|
|
Hercules |
16h 29m 24.7s |
+28° 10′ 30″ |
0 |
|
|
2218 |
|
|
Draco |
16h 35m 54.0s |
+66° 13′ 00″ |
4 |
II |
Exhibits gravitational lensing. |
2256 |
|
|
Ursa Minor |
17h 03m 43.5s |
+78° 43′ 03″ |
2 |
II-III |
|
2261 |
|
|
Hercules |
17h 22m 28.34s |
+32° 09′ 12.67″ |
|
I |
Part of the Cluster Lensing And Supernova survey with Hubble (CLASH) survey. |
2319 |
|
|
Cygnus |
19h 20m 45.3s |
+43° 57′ 43″ |
1 |
II-III |
Very close to, and possibly extending into, Lyra. |
2384 |
|
|
Capricornus |
21h 52m 18.9s |
−19° 34′ 42″ |
1 |
II-III |
|
2390 |
|
|
Pegasus |
21h 53m 34.6s |
+17° 40′ 11″ |
1 |
|
|
2440 |
|
|
|
22h 23m 52.6s |
−01° 35′ 47″ |
0 |
II |
|
2589 |
|
|
Pegasus |
23h 24m 00.5s |
+16° 49′ 29″ |
0 |
I |
|
2666 |
|
|
|
23h 50m 56.2s |
+27° 08′ 41″ |
0 |
I |
|
2667 |
|
|
Sculptor |
23h 51m 47.1s |
−26° 00′ 18″ |
3 |
I |
Exhibits strong gravitational lensing. |
2744 |
Pandora’s Cluster |
|
Sculptor |
00h 14m 19.5s |
−30° 23′ 19″ |
3 |
III |
It seems to have formed from four different clusters involved in a series of collisions over a period of some 350 million years.[6] |
3128 |
Shapley 20 Cluster |
|
|
03h 30m 34.6s |
−52° 33′ 12″ |
3 |
I-II |
|
3158 |
Shapley 17 Cluster |
|
|
03h 42m 39.6s |
−53° 37′ 50″ |
2 |
I-II |
|
3266 |
|
Horologium Supercluster |
Reticulum |
04h 31m 11.9s |
−61° 24′ 23″ |
2 |
I-II |
|
3341 |
|
|
|
05h 25m 35.1s |
−31° 35′ 26″ |
2 |
II |
|
3363 |
|
|
|
05h 45m 07.8s |
−47° 56′ 52″ |
3 |
I |
|
3526 |
Centaurus Cluster |
Hydra-Centaurus Supercluster |
Centaurus |
12h 48m 51.8s |
−41° 18′ 21″ |
0 |
I-II |
|
3558 |
Shapley 8 Cluster |
Shapley Supercluster |
|
13h 27m 54.8s |
−31° 29′ 32″ |
4 |
I |
|
3562 |
|
Shapley Supercluster |
|
13h 33m 31.8s |
−31° 40′ 23″ |
2 |
I |
|
3565 |
|
Hydra-Centaurus Supercluster |
|
13h 36m 39.9s |
−33° 58′ 17″ |
1 |
I |
|
3574 |
|
Hydra-Centaurus Supercluster |
|
13h 49m 09.4s |
−30° 17′ 54″ |
0 |
I |
|
3581 |
|
Hydra-Centaurus Supercluster |
|
14h 07m 27.5s |
−27° 01′ 15″ |
0 |
I |
|
3627 |
Norma Cluster |
|
Norma |
16h 15m 32.8s |
−60° 54′ 30″ |
1 |
I |
|
3677 |
|
|
Microscopium |
20h 26m 21s |
−33° 21′ 06″ |
|
|
possible member of Microscopium Supercluster |
3693 |
|
|
Microscopium |
20h 34m 22s |
−34° 29′ 40″ |
|
|
possible member of Microscopium Supercluster |
3695 |
|
Microscopium Supercluster |
Microscopium |
20h 34m 48s |
−35° 49′ 39″ |
|
|
gravitationally bound to Abell 3696 |
3696 |
|
Microscopium Supercluster |
Microscopium |
20h 35m 10s |
−34° 54′ 36″ |
|
|
gravitationally bound to Abell 3695 |
3705 |
|
|
Microscopium |
20h 41m 42s |
−35° 14′ 00″ |
|
|
possible member of Microscopium Supercluster |
3854 |
|
|
|
22h 17m 42.9s |
−35° 42′ 58″ |
3 |
II |
|
4059 |
|
|
|
23h 56m 40.7s |
−34° 40′ 18″ |
1 |
I |