Titlebook: Confrontation of Cosmological Theories with Observational Data; M. S. Longair Book 1974 The International Astronomical Union 1974 Big Bang

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BYRE

Confrontation of Lemaître Models and the Cosmological Constant with Observationsmological constant if non-zero must be in absolute value less than 2 × 10. cm.. The predictions of the Lemaître models are compared with modern observations. It is shown that Lemaître models without evolution fail to reproduce the observed radio source counts. The existence of quasars with large red

Agronomy

The Hubble Constant and the Deceleration Parameterheids, brightest stars, II regions, and luminosity classes) the distance scale is carried beyond any possible local anisotropy of the velocity field. Special care is taken to allow for the dependence of the intrinsic properties of the distance indicators on the size of the parent galaxy, and for the

deforestation

Evidence for Non-Velocity Redshiftsin distance, to our own. It is possible that all QSRs originate from galaxies of much lower redshift. It is shown that in the four cases where QSRs fall projected closest to bright galaxies, that in all four cases the galaxies show evidence of physical interaction. Evidence for high redshift, compac

Fracture

否决

The Counts of Radio Sourceses, we must look at . the counts of radio sources at . frequencies; second, when we attempt to evaluate the implications of the source counts, we should use proper cosmological models and not rely on the local Euclidean model.

否决

Radio Source Counts at Centimetre Wavelengthsppear to differ markedly from an integral number-flux relation having a slope of −1.5 between 5 and 5 × 10. sources per steradian, and show a sharp drop at source densities smaller then 5 sr.. On the basis of the form of the number counts and the observed anisotropies in the distribution of sources

TRAWL

Observational Foundations of Inhomogeneous Universealysed..The results of the analysis show that there is a significant non-random surface distribution of galaxies irrespective of the scale of the field investigated. The observed clumpiness does not allow us to introduce discrete hierarchical structures. The distribution of galaxies shows rather a c

FLAX

Field Galaxies and Cluster Galaxies: Abundances of Morphological Types and Corresponding Luminosity of selection probabilities, and (iii) of ‘space luminosity functions’. Strictly, the theory applies to ‘homogeneous classes’ of galaxies. This term designates a category of galaxies, say ., so finely defined that the probability, say .(. | .), that a galaxy of category . will be included in the cata

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Large Scale Anisotropy of the Cosmic Microwave Background origin. Measurements of the spectrum of the radiation, discussed earlier in this volume by Blair, are consistent with the idea that the radiation is in fact a relic of a hot, dense, initial state of the Universe — the Big Bang. If the radiation is cosmological, measurements of both its spectrum and