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December 17, 2002Astronomy and AstrophysicsOpen Access

XMM-Newton confirmation of soft X-ray excess emission in clusters of galaxies – The discovery of O VII emission from an extended warm baryonic component

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A 2002 study studied this question.

synapsesocial.com/papers/6a7d290ef1daba58ecd5a927 https://doi.org/10.1051/0004-6361:20021514

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Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Nonthermal X‐Ray Emission: An Alternative to Cluster Cooling Flows?2002 · 8 citations
2Hard X-Ray Radiation in the Coma Cluster Spectrum1999 · 260 citations
3Diffuse Extreme-Ultraviolet Emission from the Coma Cluster: Evidence for Rapidly Cooling Gases at Submegakelvin Temperatures1996 · 149 citations
4A Catalog of Soft X‐Ray Shadows, and More Contemplation of the \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 $\frac{1}{4}$ \end{document} keV Background2000 · 116 citations
5A Possible Intracluster Origin for the Excess Soft X-ray Component in Some Clusters1997 · 31 citations