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X-ray Morphology of Clusters of Galaxies and its Application

Published online by Cambridge University Press:  01 August 2006

Y. Hashimoto ,
H. Boehringer ,
J. P. Henry ,
G. Hasinger  and
G. Szokoly
Y. Hashimoto
Affiliation:
Max-Planck-Isntitut fuer extraterestrische Physik, Garching, Germany email: hashimot@mpe.mpg.de
H. Boehringer
Affiliation:
Max-Planck-Isntitut fuer extraterestrische Physik, Garching, Germany email: hashimot@mpe.mpg.de
J. P. Henry
Affiliation:
Institute of Astronomy, University of Hawaii 2680 Woodlawn Dr. Honolulu, HI 96822, USA
G. Hasinger
Affiliation:
Max-Planck-Isntitut fuer extraterestrische Physik, Garching, Germany email: hashimot@mpe.mpg.de
G. Szokoly
Affiliation:
Max-Planck-Isntitut fuer extraterestrische Physik, Garching, Germany email: hashimot@mpe.mpg.de
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Abstract

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We report our study of X-ray cluster morphology using a sample of 101 clusters of galaxies at redshift z~0.05-1 taken from the Chandra archive.

Keywords

galaxies: clusters: generalX-rays: galaxies: clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 203
Copyright
Copyright © International Astronomical Union 2007

References

Hashimoto, Y., Boehringer, H., Henry, J.P. 2006, ApJ (in press).Google Scholar