Chemical enrichment of cool-core clusters of galaxies

Details Chemical enrichment of cool-core clusters of galaxies Chemical enrichment of cool-core clusters of galaxies

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...58d&link_type=abstract

XMM-Newton Proposal ID #04015202

Statistics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Abell 262, Abell 2052, Xmm-Newton Proposal 04015202

Scientific paper

We propose to observe the clusters of galaxies Abell 262 and Abell 2052 each for 130 ks. The excellent statistics of the RGS and EPIC spectra will allow us to accurately measure the elemental abundances, like oxygen, silicon, sulfur and iron, and determine their spatial distribution. Using the measured abundances we will test theoretical supernova yields and deduce the chemical enrichment history of these clusters.

Affiliated with

Also associated with

No associations

Rating

Chemical enrichment of cool-core clusters of 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 Chemical enrichment of cool-core clusters of galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical enrichment of cool-core clusters of galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1659829