Hydra Cluster | |
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Central region of Abell 1060 (Hydra Cluster) with legacy surveys. The bright stars are HD 92036 (middle left) and HD 91964 (bottom) | |
Observation data (Epoch J2000) | |
Constellation(s) | Hydra |
Right ascension | 09h 18.0m[1] |
Declination | −12° 05′[1] |
Number of galaxies | 157[2] |
Richness class | 1[3] |
Bautz–Morgan classification | III[3] |
Redshift | 0.0548 (16,452 km/s)[1] |
Distance (co-moving) | 58.3 Mpc (190.1 Mly) h−10.705 |
X-ray flux | 6.1×10−11 erg s−1 cm−2 (0.5–2 keV)[1] |
Other designations | |
Abell 1060 | |
The Hydra Cluster (or Abell 1060) is a galaxy cluster that contains 157 bright galaxies, appearing in the constellation Hydra.[4] The cluster spans about ten million light-years and has an unusually high proportion of dark matter.[5] The cluster is part of the Hydra–Centaurus Supercluster located 158 million light-years from Earth. The cluster's largest galaxies are elliptical galaxies NGC 3309 and NGC 3311 and the spiral galaxy NGC 3312 all having a diameter of about 150,000 light-years.[6] In spite of a nearly circular appearance on the sky, there is evidence in the galaxy velocities for a clumpy, three-dimensional distribution.[7]
Coordinates: 10h 36.9m 00s, −27° 32′ 00″
Original source: https://en.wikipedia.org/wiki/Hydra Cluster.
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