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Information × Registration Number 0215U004354, 0111U006170 , R & D reports Title Characteristics of matter distribution in the Universe and properties of objects located on cosmological distances. popup.stage_title Head Zhdanov V.I., Registration Date 06-03-2015 Organization Taras Shevchenko Kiev university popup.description2 Analyzed restrictions on combinations of cosmological parameters derived from observations of the peculiar velocities of flat galaxies catalog RFGC. The obtained values of the orbital mass groups of galaxies in the Local volume with a radius of 8 IPC, which give the relationship a dark mass to glow, which is 33;this indicates a possible local deficits matter. The effect of magnetic fields on the propagation of cosmic rays from sources in the Local ndscaping. It is shown that the number of recorded events in the Auger experiment can vdovy cosmic rays accelerated in the vicinity of Centaurus A. The mechanisms of influence of cosmic rays on the content characteristics of aerosols in the earth's atmosphere, as well as the influence of the movements of air masses on the dynamics of aerosols over the place of observation, in particular over Kiev. On the material of the new sample of 52 bright compact defined the rate of star formation for radiation in the emission lines of H-alpha in the areas of ionized hydrogen and radaronline at 1.4 GHz. The estimates of the rate of star formation in close galaxies counterpart in the context of a possible dependence of the process on the density of the environment. Carried out the reduction of new data space mission INTEGRAL of the Seyfert galaxies NGC 4945. Based on the modeling of the light curves in gravitational lens systems, for a number of parameters of the optical density evaluated the accuracy of the observations necessary to determine the type of source in gravitational lens systems. Conducted teoretyczny analysis and classification rosv Azniv equations of relativistic cosmology in the framework of homogeneous isotropic models Vsesvit.Rosalina questions relativistic astrometry in weak gravitational fields. The results are of interest for extragalactic astronomy, astrophysics and cosmology, as well as climatology, they are used in the educational process (updating of courses, training manuals, work with graduate students and students.) Product Description popup.authors Іващенко Г.Ю. Ізотова І.Ю. Александров О.М. Данилевський В.О. Кудря Ю.М. Парновський С.Л. Слюсар В.М Тимчку О.О. Федорова О.В. popup.nrat_date 2020-04-02 Close