Physics
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..179v&link_type=abstract
XMM-Newton Proposal ID #04048401
Physics
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Mkw 2, Xmm-Newton Proposal 04048401
Scientific paper
The central regions of galaxy clusters, frequently occupied by massive elliptical galaxies with strong radio sources interacting with dense, X-ray emitting gas, are among the most interesting and physically active regions in the Universe, and they have been extensively studied with contemporary X-ray observatories. We here propose a deep observation of an exceptional object at the low end of the cluster mass range, MKW 2, a rich galaxy group centered on a cD that exhibits remarkably strong radio jets extending 400 kpc, a scale unusual even in massive clusters. We will examine the interaction between cluster gas and radio source, measure the properties of the gas, and examine the nature of the temperature and abundance distributions.
No associations
LandOfFree
Strong radio jets in a rich group: how disturbed is the hot gas in MKW 2? 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 Strong radio jets in a rich group: how disturbed is the hot gas in MKW 2?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Strong radio jets in a rich group: how disturbed is the hot gas in MKW 2? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1660023