The Nature of the Large Scale X-ray Emission around Abell Clusters

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Soltan et al. (1996) found a significant positive component extending up to several degrees in their angular cross-correlation function (CCF) between the ROSAT All-Sky Survey (RASS) diffuse soft X-ray (E ~ 1keV) map and Abell clusters. To explain this, one model they have suggested consists of a 20h50(-1) Mpc-scale X-ray emitting hot gas halo associated with each Abell cluster. In order to constrain the nature of this extended component, we have made CCF studies between Abell clusters and hard X-ray maps observed with HEAO-1 A2 as well as the microwave map observed with COBE DMR. Our preliminary analysis shows that there also exists an extended component in the hard X-ray - Abell cluster CCF at a similar scale, indicating that the spectrum of the extended component is harder than a thermal spectrum for gas temperatures of typical clusters. A robust upper limit to the Sunyaev-Zel'dovich decrement set by the COBE DMR - Abell cluster CCF excludes an extended gas halo model with temperatures kT>1 keV. Combining these results, we can rule out any gas origin with a smooth profile for the extended component. A possibility consistent with the data is that X-ray emitting field AGNs clustered with Abell clusters give rise to the extended CCF signal.

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

The Nature of the Large Scale X-ray Emission around Abell Clusters 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 The Nature of the Large Scale X-ray Emission around Abell Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Nature of the Large Scale X-ray Emission around Abell Clusters will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1174520

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