Galaxy properties in low X-ray luminosity clusters atz=0.25-Reference-Cited by-同舟云学术

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Galaxy properties in low X-ray luminosity clusters atz=0.25

Published:2002-11 Issue:1 Volume:337 Page:256-274
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Balogh Michael,Bower R. G.,Smail Ian,Ziegler B. L.,Davies Roger L.,Gaztelu A.,Fritz Alexander

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/337/1/256/18165599/337-1-256.pdf

Reference84 articles.

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

2. Physical implications of the X-ray properties of galaxy groups and clusters

3. Star Formation in Cluster Galaxies at 0.2 < [CLC][ITAL]z[/ITAL][/CLC] < 0.55

4. The Dependence of Cluster Galaxy Star Formation Rates on the Global Environment

5. Differential Galaxy Evolution in Cluster and Field Galaxies 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 $z\approx 0.3$ \end{document}

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1. The HectoMAP Cluster Survey: Spectroscopically Identified Clusters and their Brightest Cluster Galaxies (BCGs);The Astrophysical Journal;2021-12-01

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