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Article Contents
1 Introduction
2 Soft X-ray emissivity due to charge-exchange processes at interfaces between partially neutral IS clouds and hot gas: Comparisons with hot gas emissivity
3 Type Ia supernova remnant in the Sedov phase
4 Galactic winds and halo cold clouds
5 High velocity clouds in the galactic halo
6 Galaxy clusters and cooling flows
7 Conclusions
References

List of figures

Copyright ESO 2004
Published by EDP Sciences