The X-ray surface brightness profiles of hot galaxy clusters up to $\vec z$ ~ 0.8: Evidence for self-similarity and constraints on $\Omega

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

Published:2002-06-14 Issue:1 Volume:389 Page:1-18
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Arnaud M.,Aghanim N.,Neumann D. M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20020378/pdf

Reference83 articles.

1. Mass‐Temperature Relation of Galaxy Clusters: A Theoretical Study

2. The impact of cooling flows on the TX-LBol relation for the most luminous clusters

3. The relationship between cooling flows and metallicity measurements for X-ray-luminous clusters

4. The X-ray virial relations for relaxed lensing clusters observed withChandra

5. The LX--T relation and intracluster gas fractions of X-ray clusters

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