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Multi-Wavelength Study of Rosat Clusters of Galaxies

  • A. D. Reid (a1) (a2), R. W. Hunstead (a1) (a2) and M. M. Pierre (a1) (a2)

Extract

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).

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References

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Gregorini, L., de Ruiter, H.R., Parma, P., Sadler, E.M., Vettolani, G. & Ekers, R.D. (1994), A&AS , 106, 1.
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.
Pierre, M., Hunstead, R., Reid, A. and 10 others (1994a), ESO Messenger , 78, 24.
Pierre, M., Buhringer, H., Ebeling, H., Voges, W., Schuecker, P., Cruddace, R. & MacGillivray, H. (1994b), A&A , 290, 725.

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