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The Fate of Intra-Group Medium

Published online by Cambridge University Press:  25 May 2016

Yuhri Ishimaru*
Affiliation:
National Astronomical Observatory, 2-21-1, Mitaka, Osawa, Tokyo 181, Japan. email: ishimaru@th.nao.ac.jp

Abstract

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Combining X-ray data for clusters of galaxies, groups, and elliptical galaxies, we have obtained the evidence for that groups eject parts of the intra-group medium (IGM) via supernovae-driven ‘group winds’ like ellipticals. This scenario is confirmed by 1D hydrodynamical simulations.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Copyright
Copyright © Kluwer 1998 

References

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