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Series of galaxy clusters From Wikipedia, the free encyclopedia
The Leo II Groups, or Leo II Cloud, are a series of at least 110 galactic clusters and individual galaxies stretching approximately 30 Mly (9.2 Mpc) ecliptic west of the edge of the Virgo cluster.[1][2] It is located approximately 65 Mly (20 Mpc) to 95 Mly (29 Mpc) from the Solar System, at a right ascension of 10h 00m to 11h 40m .[1]
Leo II Groups | |
---|---|
Observation data (Epoch ) | |
Right ascension | 10h 00m to 11h 40m |
Declination | 0° to +35° |
Number of galaxies | at least 110 |
Parent structure | Virgo Supercluster |
Distance | 65 Mly (20 Mpc) to 95 Mly (29 Mpc) |
Other designations | |
Leo II Cloud | |
References: [1] |
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