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The role of diffuse matter in galactic coronas
Authors:A Chernin  J Einasto  E Saar
Institution:(1) A. Ioffe Institute of Physics and Technology, Leningrad, U.S.S.R.;(2) W. Struve Astrophysical Observatory, Estonia, U.S.S.R.
Abstract:An upper limit to the gas content in the coronas of giant galaxiesM gas<0.04M cor has been calculated on the basis of observational data on the emission of clusters of galaxies in different wavelength ranges. An analysis of companion galaxies has revealed a correlation of their morphological types with the distances to central giant galaxies. A gasodynamical interpretation of this regularity is suggested and a possible picture of the evolution of the galactic coronas is presented.
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