Formation of Starburst Galaxies in Merging Clusters

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2

Scientific paper

A significant fraction of clusters of galaxies are observed to have substructure, which implies that merging between clusters and subclusters is a rather common physical process in cluster formation. It still remains unclear how cluster merging affects the evolution of cluster member galaxies. We report the results of numerical simulations that show the dynamical evolution of a gas-rich, late-type spiral in a merger between a small group of galaxies and a cluster. The simulations demonstrate that the time-dependent tidal gravitational field during merging excites non-axisymmetric structure of the galaxy, subsequently drives efficient transfer of gas to the central region and finally triggers a secondary starburst. This result provides a close physical relationship between the emergence of starburst galaxies and the formation of substructure in clusters. We accordingly interpret post-starburst galaxies located near substructure of the Coma Cluster as one observational example indicating the global tidal effects of group-cluster merging. Our numerical results further suggest a causal link between the observed excess of blue galaxies in distant clusters and the cluster virialization process through hierarchical merging of subclusters.

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

Formation of Starburst Galaxies in Merging 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 Formation of Starburst Galaxies in Merging Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of Starburst Galaxies in Merging Clusters will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1005539

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