The role of diffuse matter in galactic coronas

Details The role of diffuse matter in galactic coronas The role of diffuse matter in galactic coronas

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..39...53c&link_type=abstract

Astrophysics and Space Science, vol. 39, Jan. 1976, p. 53-64.

Astronomy and Astrophysics

Astrophysics

9

Coronas, Galactic Clusters, Galactic Radiation, Galactic Structure, Gaseous Diffusion, Astronomical Models, Cosmology, Gas Dynamics, Luminous Intensity

Scientific paper

An upper limit to the gas content in the coronas of giant galaxies with the gas mass less than 0.04 times the core mass has been calculated using observational data on the emission from clusters of galaxies in different wavelength ranges. Analysis of companion galaxies has revealed a correlation of their morphological types with the distances to central giant galaxies. A gasdynamic interpretation of this regularity is suggested, and a possible picture of the evolution of the galactic coronas is presented.

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