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Galaxy Clusters and the Butcher-OemlerEffect:

Galaxy Transformation by Environment



                                       Emily Cross and Kristine Salters
“Like cities, each cluster has
 unique characteristics and
 population demographics:
 Coma, Virgo, and the Local
 Group are as different from
 each other as
 Toronto, Bangkok, and Rio de
 Janeiro”            (S&T: January 1988, page 16).
Galaxy cluster with high redshift have a

    higher blue star forming spiral population



    Low redshift, low blue spiral population

RED SHIFT
Infalling spiral galaxy




            Galaxy cluster
Merging

    Starburst

                              The youths
    Ram pressure stripping

    Tidal disruption





    SF completely exhausted
We had never seen the phase between the

    young blue spirals and the old red ellipticals
    until November
    of 2008
Photo

The evolving properties of
galaxies in clusters offer a unique
opportunity to connect evolution
on scales ranging from individual
galaxies to overall cosmic
evolution

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Galaxy transformation by Environment

  • 1. Galaxy Clusters and the Butcher-OemlerEffect: Galaxy Transformation by Environment Emily Cross and Kristine Salters
  • 2. “Like cities, each cluster has unique characteristics and population demographics: Coma, Virgo, and the Local Group are as different from each other as Toronto, Bangkok, and Rio de Janeiro” (S&T: January 1988, page 16).
  • 3. Galaxy cluster with high redshift have a  higher blue star forming spiral population Low redshift, low blue spiral population 
  • 4.
  • 5.
  • 7. Infalling spiral galaxy Galaxy cluster
  • 8. Merging  Starburst  The youths Ram pressure stripping  Tidal disruption  SF completely exhausted
  • 9. We had never seen the phase between the  young blue spirals and the old red ellipticals until November of 2008
  • 11. The evolving properties of galaxies in clusters offer a unique opportunity to connect evolution on scales ranging from individual galaxies to overall cosmic evolution