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X-ray Morphology of Clusters of Galaxies

Published online by Cambridge University Press:  30 March 2016

H. Böhringer ,
R.A. Schwarz ,
U.G. Briel ,
H. Ebeling  and
W. Voges
H. Böhringer
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik 8046 Garching, Germany
R.A. Schwarz
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik 8046 Garching, Germany
U.G. Briel
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik 8046 Garching, Germany
H. Ebeling
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik 8046 Garching, Germany
W. Voges
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik 8046 Garching, Germany

Abstract

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The ROSAT observatory with its high spatial resolution X-ray telescope is an ideal instrument for the study of clusters of galaxies. In the first part of the mission an All Sky X-ray Survey was conducted with ROSAT. Here we present first results of observations of Virgo, Perseus and some other clusters of galaxies from the All Sky Survey. These data illustrate the capabilities of the ROSAT observatory for studies of the morphological structure and physical properties of galaxy clusters.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 9: Highlights of Astronomy. As presented at the XXIst General Assembly of the IAU, 1991 , 1992 , pp. 205 - 209
Copyright
Copyright © Kluwer 1992

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