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0215U004225,
0112U001750
,
Study of physics of stars, galactic constituents and their gravitational fields for testing of evolution of Galaxy and Universe.
Mishenina Tamara Vasylivna,
17-02-2015
Odessa I.I.Mechnikov National University
The detailed researches of abundances of elements were carried out in stars of thin and thick disks, nearest galaxies-satellites SMC and BMC, and separate structures of disk and halo Galaxy – open and globular clusters, moving groups and other, taking into account the changes of chemical composition, connected with evolutional changes, and also results of research of physical terms in stars on the different evolutional stages. Comparing with the theories of nucleosynthesis and the models of chemical evolution was carried out. The models of transference of matter in the double systems (including Beta Lyres) are built by the own methods of three-dimensional numerical hydrodynamics. All gas structures in this system are included in a model; the model of standing shock wave, which arises up as a result of collision of winds from two component of the system, is built. The problem aspects of multidimensional models of Kaluza-Klein are considered and discovered physical reasons of these problems. It is showed that simple and most natural generalization of astrophysical objects, as our Sun, on a multidimensional case contradict to the known gravity tests in the planetary system. Mechanical approach is offered, that allows to describing the dynamics of objects (galaxies, dwarf galaxies, clusters of galaxies), taking into account, both gravity interaction of these objects and cosmological expansion.
Басак Н.Ю.
Белік С.І.
Бриленков М.Д.
Бургазлi А.В.
Гарбузов Г.О.
Гопка В.Ф.
Горбаньова Т.І.
Жук О. I.
Ковтюх В.В.
Коротін С.А.
Кудинова А.В.
Назаренко В.В.
Назаренко С.В.
Парамонова О.П.
Фахр С.Х.
Чепiжко О.О.
Чехонадських Ф.А.
Чинарова Л.Л.
Чоповський О.В.
Ющенко В.О.
2020-04-02
Updated: 2025-12-08
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