Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters

Details Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters

2008-07-16

arxiv.org/abs/0807.2605v1

Astronomy and Astrophysics

Astrophysics

5 pages, 2 figures, IAU Symposium 254

Scientific paper

The mass reinserted by young stars of an emerging massive compact cluster shows a bimodal hydrodynamic behaviour. In the inner part of the cluster, it is thermally unstable, while in its outer parts it forms an out-blowing wind. The chemical homogeneity/inhomogeneity of low/high mass clusters demonstrates the relevance of this solution to the presence of single/multiple stellar populations. We show the consequences that the thermal instability of the reinserted mass has to the galactic super-winds.

Affiliated with

Also associated with

No associations

Rating

Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters 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 Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-661016