The X-ray surface brightness profiles of hot galaxyclusters up to $\vec z$ ~ 0.8: Evidence for self-similarity andconstraints on $\Omega_\mathsf{0}$

Publisher： Edp Sciences

E-ISSN： 1432-0746|389|1|1-18

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.389, Iss.1, 2002-07, pp. : 1-18

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