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Home All issues A&A, 437 1 (2005) 31-38 Article references

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Cited article:

The impact of baryons on the sparsity of simulated galaxy clusters from THE THREE HUNDRED Project

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ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. III. MEASUREMENT BIASES AND COSMOLOGICAL EVOLUTION OF GAS AND STELLAR MASS FRACTIONS

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Mass and pressure constraints on galaxy clusters from interferometric Sunyaev–Zel'dovich observations

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Testing for evolution in scaling relations of galaxy clusters: cross analysis between X-ray and SZ observations

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Astronomy & Astrophysics 533 A45 (2011)
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Baryon fractions in clusters of galaxies: evidence against a pre-heating model for entropy generation

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Monthly Notices of the Royal Astronomical Society 413 (1) 691 (2011)
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Sunyaev-Zel’dovich galaxy clusters number counts: consequences of cluster scaling-law evolution

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Astronomy & Astrophysics 524 A81 (2010)
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Planetary companions around the K giant stars 11 Ursae Minoris and HD 32518

M. P. Döllinger, A. P. Hatzes, L. Pasquini, E. W. Guenther and M. Hartmann
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Evidence for Line‐of‐Sight Structure in a Comparison of X‐Ray and Optical Observations of the High‐Redshift Cluster RCS 043938‐2904.7

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CONFIRMATION OF THE EXOPLANET AROUND β GEM FROM THE RV OBSERVATIONS USING BOES

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Why Do Only Some Galaxy Clusters Have Cool Cores?

Jack O. Burns, Eric J. Hallman, Brennan Gantner, Patrick M. Motl and Michael L. Norman
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ChandraX‐Ray Observations of the 0.6 A. K. Hicks, E. Ellingson, M. Bautz, et al.
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Gas mass fraction fromXMM-NewtonandChandrahigh redshift clusters and its use as a cosmological test

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Revisiting the baryon fractions of galaxy clusters: a comparison with WMAP 3-yr results

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A Multiwavelength Analysis of the Strong Lensing Cluster RCS 022434‐0002.5 at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=0.778$ \end{document}

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Anatomy of a Flaring Proto-Planetary Disk Around a Young Intermediate-Mass Star

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Multi-frequency analysis of neutralino dark matter annihilations in the Coma cluster

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