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

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Observational Foundations of Inhomogeneous Universety levels and the number-flux density relations vary from place to place in the GB region and the significance level of the observed variations is at least 1%..The most important conclusion which can be drawn from the GB data is that results obtained from the observations of a single selected region
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Field Galaxies and Cluster Galaxies: Abundances of Morphological Types and Corresponding Luminosity s class..In order to validate the theory empirically, calculations were performed to predict the abundances of eight combinations of morphological types among cluster galaxies listed in the HMS Catalogue, each combination being treated as a distinct homogeneous class. Additional hypotheses underlyin
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The Thermal History of the Universe and the Spectrum of Relic Radiationns of the spectrum of the relic radiation. The absence of noticeable deviations from the Planckian spectrum enables us to set limits to the energy release in the early Universe (10. < z < 10.). But in order to have a clear picture of possible distortions, let us first review the idealized situation.
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