Open, Massive and Globular Clusters - Part of the same family?

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5 pages, 2 figures. To appear in the proceedings of IAU Symp. 207, "Extragalactic Star Clusters", eds. Grebel, Geisler, Minnit

Scientific paper

Populations of young star clusters show significant differences even among "normal" disk galaxies. In this contribution I discuss how properties of young cluster systems are related to those of their host galaxies, based on a recent study of clusters in a sample of 22 nearby spiral galaxies. Luminous young clusters similar to the "super" star clusters observed in starbursts and mergers exist in several of these galaxies, and it is found that the luminosity of the brightest star cluster as well as the specific luminosity of the cluster systems both correlate well with the host galaxy star formation rate. When considering star clusters in different environments the traditional distinction between "open", "massive" and "globular" clusters breaks down, underscoring the need for a universal physical description of cluster formation.

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

Open, Massive and Globular Clusters - Part of the same family? 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 Open, Massive and Globular Clusters - Part of the same family?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Open, Massive and Globular Clusters - Part of the same family? will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-313220

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