Effect of Environment on the Underlying Stellar Populations of Dwarf Elliptical Galaxies in the Coma Cluster

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Galaxy Clusters, Infall, Accretion, And Accretion Disks, Star Formation

Scientific paper

We derive ages, metallicities and [α/Fe] ratios for dwarf early-type galaxies (dE/dS0) in the center and a region believed to be infalling into the Coma cluster. We find that a set of metallic indices cannot be described by linear relations with velocity dispersion (σ), while another group of indices exhibits linear index-σ relations. dE/dS0 galaxies in the core of the cluster are on average younger, and have lower metallicities and lower α-ratios (solar to sub-solar) than the more luminous elliptical galaxies. On the other hand, dEs/dS0s in the infall region of Coma form a less homogeneous population. We find an unusually high fraction of dE/dS0s with high [α/Fe] ratios, suggesting short time scales for the star formation histories for these galaxies. Furthermore, the dE/dS0s with high α-ratios have a range of ages and metallicities implying multiple formation scenarios where some galaxies have experienced their short star formation bursts at more recent epochs.

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

Effect of Environment on the Underlying Stellar Populations of Dwarf Elliptical Galaxies in the Coma Cluster 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 Effect of Environment on the Underlying Stellar Populations of Dwarf Elliptical Galaxies in the Coma Cluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effect of Environment on the Underlying Stellar Populations of Dwarf Elliptical Galaxies in the Coma Cluster will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1109282

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