X-radiation from clusters of galaxies: Spectral evidence for a hot evolved gas

Details X-radiation from clusters of galaxies: Spectral evidence for a hot evolved gas X-radiation from clusters of galaxies: Spectral evidence for a hot evolved gas

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7632095s&link_type=abstract

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Galactic Clusters, Galactic Radiation, X Ray Sources, X Ray Spectra, Cosmic Plasma, High Temperature Gases, Iron, Oso, Proportional Counters, Thermal Radiation

Scientific paper

OSO-8 observations of the X-ray flux in the range 2-60 keV from the Virgo, Perseus, and Coma Clusters provide strong evidence for the thermal origin of the radiation, including iron line emission. The data are adequately described by emission from an isothermal plasma with an iron abundance in near agreement with cosmic levels. A power law description is generally less acceptable and is ruled out in the case of Perseus. Implications on the origin of the cluster gas are discussed.

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