Leo II (dwarf galaxy)

Leo II (dwarf galaxy) Leo II (or Leo B) is a dwarf spheroidal galaxy about 690,000 light-years away in the constellation Leo. It is one of 24 known satellite galaxies of the Milky Way. Leo II is thought to have a core radius of 178 ± 13 pc and a tidal radius of 632 ± 32 pc. It was discovered in 1950 by Robert George Harrington and Albert George Wilson, from the Mount Wilson and Palomar Observatories in California. Provided by Wikipedia
Showing 1 - 14 results of 14 for search 'Leo B', query time: 0.03s Refine Results
  1. 1
  2. 2
  3. 3
  4. 4
  5. 5
  6. 6
  7. 7
  8. 8
  9. 9
  10. 10
  11. 11
  12. 12
  13. 13
  14. 14

    Receptivity to innovation - overcoming N.I.H. by Clagett, Robert Powell

    Published 2008
    Other Authors: “…Leo B. Moore.…”
    Get full text
    Thesis