X ray morphology of clusters of galaxies

Details X ray morphology of clusters of galaxies X ray morphology of clusters of galaxies

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rrgo.conf....7b&link_type=abstract

In its Contributions to the Joint Discussion 3: Results from Rosar and GRO and Other Recent High Energy Astrophysics Missions of

Astronomy and Astrophysics

Astronomy

Galactic Clusters, Morphology, Rosat Mission, Sky Surveys (Astronomy), X Ray Astronomy, X Ray Telescopes, Galactic Structure, Spaceborne Astronomy, Spatial Resolution, Spectral Emission, Virgo Galactic Cluster

Scientific paper

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. First results of observations of Virgo, Perseus, and some other clusters of galaxies from the all sky survey, are presented. These data illustrate the capabilities of the ROSAT observatory for studies of the morphological structure and physical properties of galaxy clusters.

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