Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-29T12:41:34.301Z Has data issue: false hasContentIssue false

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: [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Ciotti, L., D'Ercole, A., Pellegrini, S., & Renzini, A. 1991, ApJ, 376, 380 CrossRefGoogle Scholar
David, L. P., Forman, W., & Jones, C. 1990, ApJ, 359, 29 CrossRefGoogle Scholar