Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-23T15:06:00.652Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
Rights & Permissions [Opens in a new window]

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.

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