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Multi-Wavelength Study of Rosat Clusters of Galaxies

Published online by Cambridge University Press:  25 May 2016

A. D. Reid ,
R. W. Hunstead  and
M. M. Pierre
A. D. Reid
Affiliation:
School of Physics, University of Sydney NSW 2006, Australia CEA/DSM/DAPNIA CE Saclay, France
R. W. Hunstead
Affiliation:
School of Physics, University of Sydney NSW 2006, Australia CEA/DSM/DAPNIA CE Saclay, France
M. M. Pierre
Affiliation:
School of Physics, University of Sydney NSW 2006, Australia CEA/DSM/DAPNIA CE Saclay, France

Extract

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We are engaged in a radio–IR-optical–X-ray study of two flux-limited samples of ROSAT clusters of galaxies south of declination −20° (Pierre et al., 1994a). One sample covers an area of 1750 deg2 in Hydra (Pierre et al., 1994b) and includes some distant (z ≈ 0.3) and X-ray luminous (LX ≈ 1045 ergs–1) clusters. The other sample derives from a volume-limited subset (nominally z ≤ 0.1) of southern X-ray clusters, which are the focus of an ESO Key Program (Guzzo et al., 1995).

Type
Radio Sources and their Environment
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 353 - 354
Copyright
Copyright © Kluwer 1996 

References

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Guzzo, L. and 26 others (1995) in Wide-Field Spectroscopy and the Distant Universe , eds. Maddox, S. J. and Aragón-Salamanca, A. (World Scientific: Singapore), p. 205.Google Scholar
Pierre, M., Hunstead, R., Reid, A. and 10 others (1994a), ESO Messenger , 78, 24.Google Scholar
Pierre, M., Buhringer, H., Ebeling, H., Voges, W., Schuecker, P., Cruddace, R. & MacGillivray, H. (1994b), A&A , 290, 725.Google Scholar