An analysis of electron distributions in galaxy clusters by means of the flux ratio of iron lines FeXXV and XXVI

Abstract

The interpretation of hard X-ray emission from galaxy clusters is still ambiguous and different models proposed can be probed using various observational methods. Here we explore a new method based on Fe line observations. Spectral line emissivities have usually been calculated for a Maxwellian electron distribution. In this paper a generalized approach to calculate the iron line flux for a modified Maxwellian distribution is considered. We have calculated the flux ratio of iron lines for the various possible populations of electrons that have been proposed to account for measurements of hard X-ray excess emission from the clusters A2199 and Coma. We found that the influence of the suprathermal electron population on the flux ratio is more prominent in low temperature clusters (as Abell 2199) than in high temperature clusters (as Coma).

arXiv comment6 pages, 3 figures, accepted for publication in A&A

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• The Radio Synchrotron Background: Conference Summary and Report
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• Non-Maxwellian electron distributions in clusters of galaxies
• Origin of Thermal and Non-Thermal Hard X-ray Emission from the Galactic Center
• An analysis of the temperature structure of galaxy clusters by means of the thermal Sunyaev-Zel'dovich effect
• Can electron distribution functions be derived through the Sunyaev-Zel'dovich effect?
• On the influence of high energy electron populations on metal abundance estimates in galaxy groups and clusters
• Empirical test for relativistic kinetic theories based on the Sunyaev-Zel'dovich effect