An improved deprojection and PSF-deconvolution technique for galaxy-cluster X-ray surface-brightness profiles-Reference-Cited by-同舟云学术

An improved deprojection and PSF-deconvolution technique for galaxy-cluster X-ray surface-brightness profiles

Published:2006-09-12 Issue:3 Volume:459 Page:1007-1019
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Croston J. H.,Arnaud M.,Pointecouteau E.,Pratt G. W.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20065795/pdf

Reference25 articles.

1. Arnaud, M. 2005, in Background Microwave Radiation and Intracluster Cosmology, ed. F. Melchiorri, & Y. Rephaeli (IOS Press) [arXiv:astro-ph/0508159]

2. The structural and scaling properties of nearby galaxy clusters

3. A High‐Resolution Study of the Hydra A Cluster withChandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling Flow

4. The distribution and morphology of X-ray-emitting gas in the core of the Perseus cluster

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