X-Ray Study of the Outer Region of Abell 2142 with Suzaku

Jun, 2011
14 pages
Published in:
  • Publ.Astron.Soc.Jap. 63 (2011) 1019
e-Print:

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Abstract: (arXiv)
We observed outer regions of a bright cluster of galaxies A2142 with Suzaku. Temperature and brightness structures were measured out to the virial radius (r200r_{200}) with good sensitivity. We confirmed the temperature drop from 9 keV around the cluster center to about 3.5 keV at r200r_{200}, with the density profile well approximated by the β\beta model with β=0.85\beta = 0.85. Within 0.4\r_{200}, the entropy profile agrees with r1.1r^{1.1}, as predicted by the accretion shock model. The entropy slope becomes flatter in the outer region and negative around r200r_{200}. These features suggest that the intracluster medium in the outer region is out of thermal equilibrium. Since the relaxation timescale of electron-ion Coulomb collision is expected to be longer than the elapsed time after shock heating at r200r_{200}, one plausible reason of the low entropy is the low electron temperature compared to that of ions. Other possible explanations would be gas clumpiness, turbulence and bulk motions of ICM\@. We also searched for a warm-hot intergalactic medium around r200r_{200} and set an upper limit on the oxygen line intensity. Assuming a line-of-sight depth of 2 Mpc and oxygen abundance of 0.1 solar, the upper limit of an overdensity is calculated to be 280 or 380, depending on the foreground assumption.
Note:
  • 14 pages, 8 figures