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A Cooling Flow Cluster at Redshift Z=0.2

Published online by Cambridge University Press:  12 April 2016

Anna Wolter ,
I.M. Gioia ,
T. Maccacaro ,
S.L. Morris ,
R. Nesci ,
G.C. Perola  and
R. Schild
Anna Wolter
Affiliation:
Harvard/Smithsonian Center for Astrophysics, Cambridge, MA
I.M. Gioia
Affiliation:
Harvard/Smithsonian Center for Astrophysics, Cambridge, MA Istituto di Radioastronomia del CNR, Bologna, Italy
T. Maccacaro
Affiliation:
Harvard/Smithsonian Center for Astrophysics, Cambridge, MA Istituto di Radioastronomia del CNR, Bologna, Italy
S.L. Morris
Affiliation:
Mount Wilson and Las Campanas Observatories, Pasadena, CA
R. Nesci
Affiliation:
Istituto Astronomico dell’Universita’, Roma, Italy
G.C. Perola
Affiliation:
Istituto Astronomico dell’Universita’, Roma, Italy
R. Schild
Affiliation:
Harvard/Smithsonian Center for Astrophysics, Cambridge, MA

Abstract

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In this paper we discuss the cluster of galaxies 1E0839.9+2938, serendipitously discovered at x-ray wavelengths. The collected data imply that this is an example of cooling flow cluster.

Type
6. Clusters of Galaxies, Cooling Flows
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 259 - 262
Copyright
Copyright © Cambridge University Press 1990

References

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