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Evidence from the HOT ISM from X-ray observations in external galaxies

Published online by Cambridge University Press:  17 September 2012

G. Trinchieri
G. Trinchieri*
Affiliation:
INAF-Osservatorio Astronomico di Brera, via Brera 28, 20121 Milano, Italy
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Abstract

The X-ray band provides a very powerful and unique way to explore the hot phase of the ISM in external galaxies. This phase has been known to exist in galaxies since the early Einstein observations, but only with recent detailed observations of objects in the local universe are we beginning to study it in detail and appreciate the importance of the hot ISM as a vehicle of chemical enrichment in different astrophysical environments. This knowledge can then be used to understand the properties of galaxies at the epoch of formation and their subsequent evolution, both in the field and in clusters.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 56: The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall? , 2012 , pp. 231 - 238
Copyright
© EAS, EDP Sciences, 2012

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