XMM-Newton Proposal 02062301

Details XMM-Newton Proposal 02062301 XMM-Newton Proposal 02062301

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..323o&link_type=abstract

XMM-Newton Proposal ID #02062301

Other

Abell 1060, Xmm-Newton Proposal 02062301

Scientific paper

Chandra observation suggests that Fe distribution in the central region of the non cD cluster A1060 is concentrated in small clouds with a scale of 10 kpc. We propose to evaluate the clumpiness in the metal distribution using this isothermal non cD cluster, and derive the precise mass of metals in clusters. The RGS spectrum in the central region with lines from various elements show us how this non-cD system has been enriched. We will also study the cause of the dark matter concentration in the core radius of 40 kpc based on the high sensitivity measurement of surface brightness and temperature. The nearly isothermal gas with smooth morphology in A1060 gives us a unique opportunity for an unambiguous study for spatial fluctuations of metallicity and temperature.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 02062301 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 XMM-Newton Proposal 02062301, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 02062301 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1173055