A High Angular Resolution View of Hot Gas in Clusters, Groups, and Galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Contribution to IAU Symposium 214 "High Energy Processes and Phenomena in Astrophysics" (6-10 August, 2002; Suzhou, China)

Scientific paper

We discuss two themes from Chandra and XMM-Newton observations of galaxies, groups, and clusters. First, we review observational aspects of cluster formation and evolution as matter accretes along filaments in A85 and A1367. We describe Chandra observations that probe the later evolutionary phases where the effects of mergers -- both subsonic and supersonic -- are observed in cluster cores as ``cold fronts'' and shocks. Second, we review the interactions between the hot, intracluster gas with relativistic plasma originating in active nuclei within the dominant galaxy at the cluster center. As examples of this interaction, we describe the radio and X-ray observations of M87 where buoyantly rising bubbles transfer energy and matter within the cluster core. We describe the Chandra observations of ZW3146 which exhibits both multiple cold fronts and relativistic plasma interactions. Finally, we describe the X-ray observations of NGC4636 where energy produced by the central AGN imprints a unique signature on the surrounding hot corona of the galaxy.

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

A High Angular Resolution View of Hot Gas in Clusters, Groups, and 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 A High Angular Resolution View of Hot Gas in Clusters, Groups, and Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A High Angular Resolution View of Hot Gas in Clusters, Groups, and Galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-73725

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