Can the Lumpy Distribution of Galaxies be reconciled with the Smooth X-ray Background?

Details Can the Lumpy Distribution of Galaxies be reconciled with the Smooth X-ray Background? Can the Lumpy Distribution of Galaxies be reconciled with the Smooth X-ray Background?

Dec 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.228.1170w&link_type=abstract

Nature, Volume 228, Issue 5277, pp. 1170-1174 (1970).

Mathematics

Logic

16

Scientific paper

The fluctuations in X-ray background intensity that would be generated by clusters or superclusters of galaxies exceed those observed. It may be that the X-ray background arises from low-luminosity objects which are distributed much more smoothly and are more numerous than bright optical galaxies. Hierarchical universe models in which the distribution of X-ray sources follows the cosmological mass distribution are ruled out.

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