Star Clusters in the Tidal Tails of Merging Pairs

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Star clusters can be found in galaxy mergers, not only in central regions, but also in the tidal debris. In both the Eastern and Western tidal tails of NGC 3256 there are dozens of young star clusters, confirmed by their blue colors and larger concentration index as compared to sources off of the tail. Tidal tails of other galaxy pairs do not have such widespread cluster formation though there are concentrations of young star clusters in the putative tidal dwarf galaxies, indicating environmental influences on the process of star formation or the packaging of the stars.

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

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

Rate now

     

Profile ID: LFWR-SCP-O-1022003

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