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Information × Registration Number 0214U002915, 0110U007860 , R & D reports Title The development and use of cluster technology for multiscale dynamical modeling and structure of the Universe popup.stage_title Head Berczik P.P., Registration Date 31-01-2014 Organization Main Astronomical Observatory popup.description2 Within the framework of project was conducted complex research and design of astrophysical tasks after three basic directions: a) the Dynamic and hydrodynamic evolution of the Galactic volume. The Dynamic and hydrodynamic evolution of the Galactic volume. We presented the new variant of multiphase хемо of dynamic koda for the evolution of galaxies. In коda we tried to decide the basic problem of all similar previous simulations, namely, shortage of dynamic permission of transition of hot gas in a cold phase. An interstellar environment we described with the use of two different phases: hot gas with the use of SPH, and cold gas with the "dense" system of particles. Stars are created only from a cold gas phase, in that time as a return of the chemically enriched matter from stars took place in both to gas phases. b) Dynamic research of evolution of the star systems in the Galactic disk. в) Dynamic research of confluence of black holes in the center of galaxies. Dynamic research of evolution of the star systems is in the Galactic disk. This year, as well as in previous years, we continued research of dynamics of star clusters( first of all analysis of loss of mass of accumulations) in the Galactic disk. A galaxy in this case was designed by the external fixed potential. We showed in-process, that initial data (namely filling of initial volume of Roshe-klaster) were an important parameter in the study of dynamic loss of mass star system. c) Dynamic research of confluence of black holes in the center of galaxies. In this year of research of dynamics and confluence of black holes in galactic kernels it is presented in three works. We investigated influence of oblate of galactic center on properties and temporal scale of confluence of central black holes in these systems. It is convincingly shown in-process, using our phi - GRAPE GPU code, that the oblate( c/a < 0.8 ) of galactic center (even without substantial of general rotatory moment) gives an opportunity of confluence of supermassive black holes on a time-scale less than 1 Gyr. From photometric data in the different ranges of waves, we classified 5142 the x-rayed point sources from the deep review of ХММ- LSS and defined the photometric red mixing for them. Among 5142 x-rayed sources it is found three perspective candidate in GLS. Empiric betweennesss are built by descriptions in optical, near infra-red and HI ranges for the isolated galaxies from a catalogue 2MIG, that embraces all sky. A complex study of selection is undertaken 117 x-rayed accumulations of galaxies from data of space observatory Chandra; cross-correlation dependences are first got between "luminescence-temperature-mass of gas" of Х- accumulations of galaxies on redshifts to 1.4; content of visible and hidden mass is got in these accumulations. Product Description popup.authors Берцик Петер Петерович Бульба Тамара Петрівна Вавилова Ірина Борисівна Веденичева Ірина Петрівна Велесь Олександр Анатолійович Елиїв Андрій Андрійович Зінченко І.А. Караченцева В. Ю. Лобортас Валентин Аскольдович popup.nrat_date 2020-04-02 Close