X-ray Imaging Spectroscopy of Abell 1835

Abstract

We present detailed spatially-resolved spectroscopy results of the observation of Abell 1835 using the European Photon Imaging Cameras (EPIC) and the Reflection Grating Spectrometers (RGS) on the XMM-Newton observatory. Abell 1835 is a luminous ($10^{46}$ ergs $s^{-1}$), medium redshift ($z=0.2523$), X-ray emitting cluster of galaxies. The observations support the interpretation that large amounts of cool gas are present in a multi-phase medium surrounded by a hot ($k{T}_e$=8.2 keV) outer envelope. We detect O VIII Ly$\alpha$ and two Fe XXIV complexes in the RGS spectrum. The emission measure of the cool gas below $k{T}_e$=2.7 keV is much lower than expected from standard cooling-flow models, suggesting either a more complicated cooling process than simple isobaric radiative cooling or differential cold absorption of the cooler gas.

6 pages, 4 figures, Accepted by A&A letters, XMM issue

References in corpus (8)

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• XMM-Newton observations of the cluster of galaxies Sersic 159-03
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• The life of central radio galaxies in clusters: AGN-ICM studies of eRASS1 clusters in the ASKAP fields
• Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• White Paper: Radio Emission and Polarization Properties of Galaxy Clusters with VLASS