Journal
ASTRONOMY & ASTROPHYSICS
Volume 365, Issue 1, Pages L104-L109Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20000021
Keywords
galaxy clusters : individual : Abell 1835; galaxies : cooling flows; techniques : spectroscopic
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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 (kT(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 kT(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.
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