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X-ray observations of the Ophiuchus, PKS 0745-191 and Cygnus-A clusters of galaxiesObservations are reported of the X-ray emission from three bright clusters of galaxies at low Galactic latitudes: the Ophiuchus, PKS 0745-191, and Cygnus-A clusters. Temperatures and iron abundances are determined from Exosat spectral data. Images of the Ophiuchus cluster show it to have a high central density and a cooling flow. Measurements of a high gas density around PKS 0745-191 and are confirmed, and it is shown that the X-ray emission is centered on the radio galaxy. The PKS 0745-191 cluster is the most distant object for which an abundance has been measured from X-ray spectra. The spectrum of Cygnus-A contains a highly absorbed power-law component that is identified with the nucleus of the radio source.
Document ID
19870059866
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Arnaud, K. A.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Johnstone, R. M.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Fabian, A. C.
(Cambridge University United Kingdom)
Shafer, R. A.
(NASA Goddard Space Flight Center Greenbelt, MA; ESA, European Space Operations Centre, Darmstadt, United States)
Mushotzky, R. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 13, 2013
Publication Date
July 1, 1987
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 227
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
87A47140
Funding Number(s)
CONTRACT_GRANT: NAS8-30751
Distribution Limits
Public
Copyright
Other

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