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Hot ISM in young elliptical galaxies

Published online by Cambridge University Press:  21 October 2010

Dong-Woo Kim
Dong-Woo Kim*
Affiliation:
Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, USA email: kim@cfa.harvard.edu
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Abstract

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Using Chandra and XMM-Newton X-ray observations of young, post-merger elliptical galaxies, we present X-ray characteristics of age-related observational results, by comparing with typical old elliptical galaxies in terms of X-ray properties of their low-mass X-ray binaries (LMXBs) and hot interstellar matter (ISM).

Keywords

galaxies: elliptical and lenticularcDX-rays: galaxiesX-rays: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 285
Copyright
Copyright © International Astronomical Union 2010

References

Kim, D.-W. & Fabbiano, G. 2004, ApJ 613, 933Google Scholar
Thomas, D., Maraston, C., Bender, R., & de Oliveira, C. M. 2005, ApJ 621, 673Google Scholar