On the Origin of Intergalactic Gas in Clusters of Galaxies and Sources of its Energy

Details On the Origin of Intergalactic Gas in Clusters of Galaxies and Sources of its Energy On the Origin of Intergalactic Gas in Clusters of Galaxies and Sources of its Energy

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988afz....28...73g&link_type=abstract

Astrofizika, Vol.28:1, P. 73, 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

The data on Fe abundances in intergalactic gas (IGG) and on mass of IGG are briefly discussed. The evolution of this abundances is considered and results of calculations are compared with the observational data on clusters of galaxies. It is found that the prevailing part of IGG consists of interstellar gas sweeped with the galactic wind from galaxies to the intergalactic space. Some consequences of this fact are mentioned, in particular, related to the problem of heating of IGG.

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