X-ray observations of the galaxy cluster PKS 0745-191: to the virial radius, and beyond

被引:105
作者
George, M. R. [1 ]
Fabian, A. C. [1 ]
Sanders, J. S. [1 ]
Young, A. J. [2 ]
Russell, H. R. [1 ]
机构
[1] Inst Astron, Cambridge CB3 0HA, England
[2] Univ Bristol, HH Wills Phys Lab, Bristol BS8 1TL, Avon, England
关键词
galaxies: clusters: general; galaxies: clusters: individual: PKS 0745-191; X-rays: galaxies: clusters; SURFACE BRIGHTNESS PROFILES; MASSIVE COOLING-FLOW; FLUX-LIMITED SAMPLE; TEMPERATURE PROFILES; XMM-NEWTON; LUMINOSITY FUNCTION; INTRACLUSTER MEDIUM; SCALING PROPERTIES; NEARBY CLUSTERS; GAS-DENSITY;
D O I
10.1111/j.1365-2966.2009.14547.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We measure X-ray emission from the outskirts of the cluster of galaxies PKS 0745-191 with Suzaku, determining radial profiles of density, temperature, entropy, gas fraction and mass. These measurements extend beyond the virial radius for the first time, providing new information about cluster assembly and the diffuse intracluster medium out to similar to 1.5 r(200) (r(200) similar or equal to 1.7Mpc similar or equal to 15 arcmin). The temperature is found to decrease by roughly 70 per cent from 0.3 to 1r(200). We also see a flattening of the entropy profile near the virial radius and consider the implications this has for the assumption of hydrostatic equilibrium when deriving mass estimates. We place these observations in the context of simulations and analytical models to develop a better understanding of non-gravitational physics in the outskirts of the cluster.
引用
收藏
页码:657 / 666
页数:10
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