Observational signatures and statistics of galaxy Cluster Mergers: Results from X-ray observations with ROSAT, ASCA, and XMM-Newton

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5

Scientific paper

In this chapter we focus on the discussion of observational data on cluster mergers. The majority of the results shown comes from observations with the ROSAT observatory. Results from ASCA, BeppoSAX and from very recent observations performed with XMM-Newton are also included. We discuss the signature and diagnostics of the merger process in galaxy clusters. We show some observable effects caused by mergers. Based on large statistically complete samples of X-ray selected galaxy clusters we consider the frequency and statistics of cluster mergers and compare them to predictions of cosmological models.

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

Observational signatures and statistics of galaxy Cluster Mergers: Results from X-ray observations with ROSAT, ASCA, and XMM-Newton 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 Observational signatures and statistics of galaxy Cluster Mergers: Results from X-ray observations with ROSAT, ASCA, and XMM-Newton, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational signatures and statistics of galaxy Cluster Mergers: Results from X-ray observations with ROSAT, ASCA, and XMM-Newton will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1893549

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