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  2. Perseus–Pisces Supercluster - Wikipedia

    en.wikipedia.org/wiki/Perseus–Pisces_Supercluster

    The Perseus–Pisces Supercluster is one of two dominant concentrations of galaxies (the other being the Local supercluster) in the nearby universe (within 300 million light years). This supercluster also borders a prominent void, the Taurus Void , and is part of the Perseus–Pegasus Filament which stretches for roughly a billion light years .

  3. Supercluster - Wikipedia

    en.wikipedia.org/wiki/Supercluster

    It consisted of two known rich clusters and one newly discovered cluster as a result of the study that discovered it. The then known clusters were Cl 1604+4304 (z=0.897) and Cl 1604+4321 (z=0.924), which then known to have 21 and 42 known galaxies respectively. The then newly discovered cluster was located at 16 h 04 m 25.7 s, +43° 14′ 44.7 ...

  4. Category:Perseus-Pisces Supercluster - Wikipedia

    en.wikipedia.org/wiki/Category:Perseus-Pisces...

    Perseus Cluster This page was last edited on 18 October 2022, at 19:42 (UTC). Text is available under the Creative Commons Attribution-ShareAlike 4.0 License ...

  5. Perseus–Pegasus Filament - Wikipedia

    en.wikipedia.org/wiki/Perseus–Pegasus_Filament

    The Perseus–Pegasus Filament is a galaxy filament containing the Perseus–Pisces Supercluster and stretching for roughly a billion light-years (or over 300/h Mpc). Currently, it is considered to be one of the largest known structures in the universe. [note 1] This filament is adjacent to the Pisces–Cetus Supercluster Complex.

  6. Alpha Persei Cluster - Wikipedia

    en.wikipedia.org/wiki/Alpha_Persei_Cluster

    The Alpha Persei Cluster, also known as Melotte 20 or Collinder 39, is an open cluster of stars in the northern constellation of Perseus. To the naked eye, the cluster consists of several blue-hued spectral type B stars. The most luminous member is the ~2nd magnitude yellow supergiant Mirfak, also known as Alpha Persei.

  7. Galaxy filament - Wikipedia

    en.wikipedia.org/wiki/Galaxy_filament

    This was the first super-large large-scale structure or pseudo-structure in the universe to be discovered. The CfA Homunculus lies at the heart of the Great Wall, and the Coma Supercluster forms most of the homunculus structure. The Coma Cluster lies at the core. [22] [23] Sloan Great Wall (SDSS Great Wall) 2003 z=0.07804 433 Mpc long

  8. Southern Supercluster - Wikipedia

    en.wikipedia.org/wiki/Southern_Supercluster

    The Southern Supercluster is a branch of a larger filament extending from the Centaurus Cluster that is known as the Southern Supercluster Strand which also encompasses the Telescopium−Grus Cloud. The Southern Supercluster Srand extends all the way to the Perseus–Pisces Supercluster .

  9. Category:Perseus Cluster - Wikipedia

    en.wikipedia.org/wiki/Category:Perseus_Cluster

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