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The Local Void is a vast, empty region of space, lying adjacent to the Local Group. [ 3 ] [ 4 ] Discovered by Brent Tully and Rick Fisher in 1987, [ 5 ] the Local Void is now known to be composed of three separate sectors, separated by bridges of "wispy filaments ". [ 4 ]
The KBC Void (or Local Hole) is an immense, comparatively empty region of space, named after astronomers Ryan Keenan, Amy Barger, and Lennox Cowie, who studied it in 2013. [1] The existence of a local underdensity has been the subject of many pieces of literature and research articles.
a map of galaxy voids. This is a list of voids in astronomy. ... Local Void: 18 h 38 m +18° cz=2500 km/s 60 Mpc [1] Northern Local Supervoid: 61 Mpc 104 Mpc
Local Sheet: 7 Mpc 2.16×10 20: Group of galaxies including the Local Group moving at the same relative velocity towards the Virgo Cluster and away from the Local Void. [40] [41] Virgo Supercluster: 30 Mpc 9.26×10 20: The supercluster of which the Local Group is a part. It comprises roughly 100 galaxy groups and clusters, centred on the Virgo ...
Largest Galaxy in the Local Group (The Milky Way is the second largest), with at least 19 satellite galaxies. ... In the Local Void [113] 202 Messier 81: SA(s)ab ...
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Di Nel la H. et al found no evidence of a connection between Pavo–Indus and the Perseus–Pisces Supercluster. [11] However, Tully et al. revealed the existence of a filamentary extension of the Pavo–Indus Supercluster known as the Arch [10] that caps the Local Void in the supergalactic north and provides a connection to the Perseus–Pisces Supercluster [14] [15] before terminating close ...
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