Star-forming galaxies in low-redshift clusters: Comparison of integrated properties of cluster and field galaxies

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9 pages, 10 figures, accepted for publication in Astronomy and Astrophysics

Scientific paper

We investigate the effect of the cluster environment on the star formation properties of galaxies in 8 nearby Abell clusters. Star formation properties are determined for individual galaxies using the equivalent width of H alpha plus [NII] line emission from narrow-band imaging. Equivalent width distributions are derived for each galaxy type in each of 3 environments - cluster, supercluster (outside the cluster virial radius) and field. The effects of morphological disturbance on star formation are also investigated. We identify a population of early-type disk galaxies in the cluster population with enhanced star formation compared to their field counterparts. The enhanced cluster galaxies frequently show evidence of disturbance, and the disturbed galaxies show marginal evidence for a higher velocity dispersion, possibly indicative of an infalling population.

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-forming galaxies in low-redshift clusters: Comparison of integrated properties of cluster and field galaxies 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-forming galaxies in low-redshift clusters: Comparison of integrated properties of cluster and field galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star-forming galaxies in low-redshift clusters: Comparison of integrated properties of cluster and field galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-697645

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