Hydra–Centaurus Supercluster
The Hydra–Centaurus Supercluster, or the Hydra and Centaurus Superclusters, was a previously defined supercluster in two parts, which prior to the identification of Laniakea Supercluster in 2014 is the closest neighbour of the former Virgo Supercluster. Its center is located about away, with it extending to a maximum distance of around.
Physical characteristics
The supercluster includes four large galaxy clusters in the Centaurus part, also known as the "4 clusters- Abell 3526
- Abell 3565
- Abell 3574
- Abell 3581
Antlia Wall
The Antlia Wall, also known as the Antlia Strand, Hydra Wall, Hydra-Antlia wall, Hydra-Antlia extension, and the Hydra-Antlia filament, is a filament that emerges from the Centaurus Cluster, passes under the Zone of Avoidance as the "Puppis filament", to link up the Lepus Cloud. This filament then passes through a region containing the NGC 1600 Group before crossing the boundary where the gravitional flows of galaxies between the Laniakea and Perseus–Pisces superclusters diverge to link up with the Perseus–Pisces supercluster at a distance of around from the Centaurus Cluster. The filament contains two major clusters:- Hydra Cluster
- Antlia Cluster
Before 2017, it was not known that the Antlia Wall and the Lepus Cloud were part of the same structure, the Centaurus–Puppis–PP Filament. This is because the Centaurus–Puppis–PP Filament goes under the ZOA of the Milky Way, which caused parts of the filament to be obscured by the disk of the galaxy on the sky, resulting in the naming of the different visible pieces of filament.
Other clusters
Apart from the central clusters, which are 150 to 200 million light years away, several smaller clusters belong to the group.Within the proximity of this supercluster lies the Great Attractor, dominated by the Norma Cluster. This massive cluster of galaxies exerts a large gravitational force, causing all matter within 50 Mpc to experience a bulk flow of 600 km/s toward the Norma Cluster.