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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. [1]

  3. NGC 1275 - Wikipedia

    en.wikipedia.org/wiki/NGC_1275

    NGC 1275 (also known as Perseus A or Caldwell 24) is a type 1.5 Seyfert galaxy [3] located around 237 million light-years away [2] in the direction of the constellation Perseus. NGC 1275 is a member of the large Perseus Cluster of galaxies.

  4. NGC 1245 - Wikipedia

    en.wikipedia.org/wiki/NGC_1245

    NGC 1245 is an open cluster in the constellation Perseus. It was discovered by William Herschel in 11 December 1786. [2] It is located 3° southwest of alpha Persei and can be spotted with 10x50 binoculars. [3] The cluster is nearly 1 billion years old. [4] NGC 1245 has about 200 members the brightest of which are of 12th magnitude. [5]

  5. 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 ...

  6. 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 ...

  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. 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.

  9. Visual field test - Wikipedia

    en.wikipedia.org/wiki/Visual_field_test

    A visual field test is an eye examination that can detect dysfunction in central and peripheral vision which may be caused by various medical conditions such as glaucoma, stroke, pituitary disease, brain tumours or other neurological deficits.

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