XMM-Newton follow-up of 3 BeppoSAX-WFC detected Clusters of Galaxies

Details XMM-Newton follow-up of 3 BeppoSAX-WFC detected Clusters of Galaxies XMM-Newton follow-up of 3 BeppoSAX-WFC detected Clusters of Galaxies

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..293g&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Computer Science

Databases

Clusters Of Galaxies, Sky Surveys, X-Ray Sources (Astronomical), Spectroscopy, Brightness, Galaxy Clusters, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., X-Ray Sources, X-Ray Bursts, Composition, Energy Spectra And Interactions, Luminosity And Mass Functions

Scientific paper

We study the physical properties of three clusters of galaxies, selected from the Bep-poSAX Wide Field Camera (WFC) survey. We obtained XMM-Newton follow-up observations for these three clusters and fit emission models to spectra obtained from the EPIC-pn. We determine the temperature, as well as the radial Fe abundances profiles. Two clusters were affected by an enhanced soft-proton background. Despite of this, we are able to classify one cluster as a cool-core cluster (kT~3.0 keV) and a another as non-cool-core cluster (kT 8.2 keV). The dimmest cluster was not classified, and has a temperature of 3.2 keV.

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