The cluster temperature has been measured using the Sunyaev-Zeldovich (SZ) effect alone, finding excellent agreement with X-ray temperature determinations. However, the galaxy clusters are not iso-thermal, and the radial temperature dependence will affect the cluster parameters derived through the observation of the SZ effect. One finds that the Compton weighted electron temperature is accurately derived through SZ observations, however, the derived peculiar velocity will be systematically shifted by 10-20%. We also address the possibility that clusters are locally only in kinetic equilibrium (not in full local thermal equilibrium), which will affect the SZ effect. (c) 2006 Elsevier B.V. All rights reserved.
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Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USAUniv Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Tsui, Lokman
Li, Zi-Xiang
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Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USAUniv Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Li, Zi-Xiang
Huang, Yen-Ta
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Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USAUniv Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Huang, Yen-Ta
Louie, Steven G.
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Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Lawrence Berkeley Natl Lab, Mat Sci Div, Berkeley, CA 94720 USAUniv Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Louie, Steven G.
Lee, Dung-Hai
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Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
Lawrence Berkeley Natl Lab, Mat Sci Div, Berkeley, CA 94720 USAUniv Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
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Department of Physics,University of CaliforniaDepartment of Physics,University of California
Zi-Xiang Li
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Yen-Ta Huang
Steven G. Louie
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Department of Physics,University of California
Materials Sciences Division,Lawrence Berkeley National LaboratoryDepartment of Physics,University of California