THE KINEMATIC OF RELATIVISTIC MOTIONS IN ASTROPHYSICAL OBJECTS - KEY TO THE VERIFICATION OF THE TIME - COORDINATE TRANSFORMATIONS

Автор(и)

  • M. G. Larionov Sternberg Astronomical Institute Moscow State University, Universitetskii Prospect 13, 119899 Moscow, Russia, Russian Federation

DOI:

https://doi.org/10.18524/1810-4215.1999.12.93088

Ключові слова:

relativity theory

Анотація

On the basis of the independent interpretation of Mickelson-Morley experiment the not Lorenz transformations were suggested. Astrophysical data on kinematic for relativistic out flows in galactic sources was investigated. It was shown that the differences between standard relativistic transformations and the suggested ones occur at the v3/c3 power. That does not allow to accept or to reject this or that kind of transformations. Peculiarities of the observational data being the result of suggested transformations were enumerated.

Посилання

Bridle A.H.: 1984, Astron. J., 89, 979.

Larionov M.G.: 1993, Astron. Tsirc., N1554, p.13.

Larionov M.G.: 1997a, in: XXVII radio astronomical conference, St. Peterburg, 1, 215.

Larionov M.G.: 1997b, Astrophys. Space Sci., 252, 140.

Larionov M.G.: 1999, in: Astrophysika na rubezhe vekov, publ. ASC FIAN, Moskow, in press.

Margon B.A.: 1984, Rev. Astr. Astrophys., 22, 507.

Parma P.: 1981, Astron. and Astrophys, 181, 244

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Опубліковано

2017-03-16

Номер

Том 12 (1999)

Розділ

Статті

Ліцензія

Авторське право (c) 2017 Odessa Astronomical Publications

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Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року