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In ], '''voids''' are the empty spaces between ], one of the largest-scale structures in the ] that contain hardly any, or no galaxies. Voids typically have a diameter of 11 to 150 ]; particularly large voids, defined by the absence of rich ]s, are sometimes called '''supervoids'''. In ], '''voids''' are the empty spaces between ], some of the largest-scale structures in the ] that contain hardly any, or no galaxies. Voids typically have a diameter of 11 to 150 ]; particularly large voids, defined by the absence of rich ]s, are sometimes called '''supervoids'''.


A ] census ("''The structure of the Universe traced by rich clusters of galaxies.''", see References) lists a total of 27 supervoids with a distance of up to 740 Mpc; a selection is given below: A ] census ("''The structure of the Universe traced by rich clusters of galaxies.''", see References) lists a total of 27 supervoids with a distance of up to 740 Mpc; a selection is given below:

Revision as of 13:36, 29 May 2005

In astronomy, voids are the empty spaces between filaments, some of the largest-scale structures in the Universe that contain hardly any, or no galaxies. Voids typically have a diameter of 11 to 150 Mpc; particularly large voids, defined by the absence of rich superclusters, are sometimes called supervoids.

A 1994 census ("The structure of the Universe traced by rich clusters of galaxies.", see References) lists a total of 27 supervoids with a distance of up to 740 Mpc; a selection is given below:

#NameDistance (Mpc)Diameter (Mpc)
1 188124
5 182130
9Southern Local Supervoid135158
18 168144
19 168152
20Bootes Void304110
21 201163
24Northern Local Supervoid86146

External links

References

  1. U. Lindner, J. Einasto, M. Einasto, W. Freudling, K. Fricke, E. Tago: The structure of supervoids. I. Void hierarchy in the Northern Local Supervoid., Astron. Astrophys., v.301, p.329 (1995)
  2. M. Einasto, J. Einasto, E. Tago, G. B. Dalton, H Andernach: The structure of the Universe traced by rich clusters of galaxies., Mon. Not. R. Astron. Soc. 269, 301 (1994)
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