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- W2587657768 endingPage "3826" @default.
- W2587657768 startingPage "3801" @default.
- W2587657768 abstract "Multi-wavelength techniques can probe the distribution and the physical properties of baryons and dark matter in galaxy clusters from the inner regions out to the peripheries. We present a full three-dimensional analysis combining strong and weak lensing, X-ray surface brightness and temperature, and the Sunyaev-Zel'dovich effect. The method is applied to MACS J1206.2-0847, a remarkably regular, face-on, massive, M_{200}=(1.1+-0.2)*10^{15}M_Sun/h, cluster at z=0.44. The measured concentration, c_{200}=6.3+-1.2, and the triaxial shape are common to halos formed in a LCDM scenario. The gas has settled in and follows the shape of the gravitational potential, which is evidence of pressure equilibrium via the shape theorem. There is no evidence for significant non-thermal pressure and the equilibrium is hydrostatic." @default.
- W2587657768 created "2017-02-17" @default.
- W2587657768 creator A5006118717 @default.
- W2587657768 creator A5013273136 @default.
- W2587657768 creator A5042382969 @default.
- W2587657768 creator A5043554110 @default.
- W2587657768 creator A5074728711 @default.
- W2587657768 creator A5081500592 @default.
- W2587657768 creator A5083570343 @default.
- W2587657768 creator A5087537882 @default.
- W2587657768 date "2017-02-07" @default.
- W2587657768 modified "2023-10-01" @default.
- W2587657768 title "CLUMP-3D: three-dimensional lensing and multi-probe analysis of MACS J1206.2−0847, a remarkably regular cluster" @default.
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