The X-ray structure of a galaxy cluster at Z = 0.54 - Implications for cluster evolution and cosmology

Details The X-ray structure of a galaxy cluster at Z = 0.54 - Implications for cluster evolution and cosmology The X-ray structure of a galaxy cluster at Z = 0.54 - Implications for cluster evolution and cosmology

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...251l..65w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 251, Dec. 15, 1981, p. L65-L68. NASA-supported research.

Astronomy and Astrophysics

Astronomy

54

Cosmology, Galactic Clusters, Galactic Evolution, X Ray Sources, Gas Evolution, High Resolution, Red Shift, X Ray Astronomy

Scientific paper

High-resolution X-ray observations of the rich cluster 0016+16 at a redshift of 0.541 are presented. The emitting gas in this cluster is hot and extremely luminous, and its structure resembles that seen in the brightest nearby cluster sources. In most of its properties, 0016+16 resembles a richer version of the Coma cluster, and it offers little support to the hypothesis that clusters at z greater than 0.5 differ fundamentally from nearer objects.

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