Evolution of galaxy cluster scaling from XMM-Newton observation of the galaxy clusters at z⩾0.4

Author:

Anokhin S.G.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference9 articles.

1. Arnaud, K.A. XSPEC: The first ten years, in: Jacoby, G.H., Barnes, J. (Eds.), Astronomical Data Analysis Software and Systems V, A.S.P. Conference Series, vol. 101, pp. 17–20, 1996.

2. XMM-NEWTON observation of the distant (z=0.6) galaxy cluster RX J1120.1+4318;Arnaud;A&A,2002

3. The structural and scaling properties of nearby galaxy clusters. II. The M—T relation;Arnaud;A&A,2005

4. XMM-NEWTON Observations of Evolution of Cluster X-ray Scaling Relations at z=0.4–0.7;Kotov;ApJ,2005

5. Chandra sample of galaxy clusters at z=0.4–0.55: Evolution in the mass-temperature relation;Kotov;ApJ,2006

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