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- W131004096 abstract "A statistical analysis of the distributions of C IV and Mg II absorption-line systems observed in quasar spectra within the cosmological redshift interval z =0 .2-3.2 is pre- sented. The results indicate that the overall z-distribution of absorbing matter is non-uniform: it has statistically significant maxima and minima, but it appears statistically isotropic. The maxima in thez-distribution of absorption systems are found at zm = 0.44, 0.77, 1.04, 1.30, 1.46, 1.60, 1.78, 1.98, 2.14, 2.45, 2.64, and 2.86 (±0.04). The positions of maxima and minima of the z-distribution turn out to be the same (within the sta- tistical uncertainty) for different celestial hemispheres indepen- dently of their orientation. The resulting space-time distribution of absorbing matter resembles successively embedded spheres corresponding to the zm values indicated. The most probable origin of such a distribution is an alternation of pronounced and depressed epochs in the course of cosmological evolution." @default.
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- W131004096 date "2000-06-01" @default.
- W131004096 modified "2023-09-23" @default.
- W131004096 title "Space-time distributions of QSO absorption systems" @default.
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