X-ray imaging-spectroscopy of Abell 1835

We present detailed spatially-resolved spectroscopy results of the observat ion 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-ra y emitting cluster of galaxies. The observations support the interpretation that large amounts of cool gas are present in a multi-phase medium surroun ded by a hot (kT(e) = 8.2 keV) outer envelope. We detect O VIII Ly alpha an d two Fe XXIV complexes in the RGS spectrum. The emission measure of the co ol gas below kT(e) = 2.7 keV is much lower than expected from standard cool ing-flow models, suggesting either a more complicated cooling process than simple isobaric radiative cooling or differential cold absorption of the co oler gas.