Metal-rich and metal-poor globular clusters in ellipticals: Did we learn anything? or Constraints on galaxy formation and evolution from globular cluster sub-populations

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Proceeding of the conference "Extragalactic Star Clusters" held in Pucon, March 12-16, 2001, eds.Grebel, Geisler, Minniti, 11

Scientific paper

A brief review on globular cluster sub-populations in galaxies, and their constraints on galaxy formation and evolution is given. The metal-poor and metal-rich sub-populations are put in a historical context, and their properties, as known to date, are summarized. We review why the study of these sub-populations is extremely useful for the study of galaxy formation and evolution, but highlight a few caveats with the current interpretations. We re-visit the current globular cluster system formation scenarios and show how they boil down to a single scenario for the metal-poor clusters (namely the formation in ``universal'', small fragments at high $z$) and that a hierarchical formation seems favored for the metal-rich clusters.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Metal-rich and metal-poor globular clusters in ellipticals: Did we learn anything? or Constraints on galaxy formation and evolution from globular cluster sub-populations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Metal-rich and metal-poor globular clusters in ellipticals: Did we learn anything? or Constraints on galaxy formation and evolution from globular cluster sub-populations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metal-rich and metal-poor globular clusters in ellipticals: Did we learn anything? or Constraints on galaxy formation and evolution from globular cluster sub-populations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-353670

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.