Variations of the quasar radio spectra with period 130 h⁻¹ Mpc
It is known that the spatial distribution of galaxies and quasars is structured at a scale LS = 130 h⁻¹Mpc. The same scale can be present at a spatial distribution of the physical characteristics of quasars. The search of period ≈ LS was conducted in the radiospectral indices of quasars in a centime...
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| Опубліковано в: : | Кинематика и физика небесных тел |
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| Дата: | 2005 |
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| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2005
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/79606 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | Variations of the quasar radio spectra with period 130 h⁻¹ Mpc / M. Khodyachikh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 71-74. — Бібліогр.: 10 назв. — англ. |
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nasplib_isofts_kiev_ua-123456789-79606 |
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| spelling |
Khodyachikh, M. 2015-04-03T15:11:53Z 2015-04-03T15:11:53Z 2005 Variations of the quasar radio spectra with period 130 h⁻¹ Mpc / M. Khodyachikh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 71-74. — Бібліогр.: 10 назв. — англ. 0233-7665 https://nasplib.isofts.kiev.ua/handle/123456789/79606 It is known that the spatial distribution of galaxies and quasars is structured at a scale LS = 130 h⁻¹Mpc. The same scale can be present at a spatial distribution of the physical characteristics of quasars. The search of period ≈ LS was conducted in the radiospectral indices of quasars in a centimetre range. The Veron-Cetti & Veron catalogue [10] was used as source. In the power spectra of series of spectral indices and proper distances of quasars the peak corresponding to the expected period confidently emerges. 0.23 ± 0.03 estimation of the parameter of density was obtained by the method of smoothing the period in different ranges of z at the varying parameter of density in the flat model of Universe. Interpretation of argument of periodicity, as proper distance, results in a geocentrism. The conformable time is proportional to proper distance and is also a good approximation of the argument of periodicity when the parameter of density equals to 0.23. At the temporal character of the exposed periodicity the centred position of the observer is not required. In such interpretation the exact expression for the argument of periodicity is unknown. The proper distance or the conformable time is introduced by its true values with an accuracy not worse than 1%. en Головна астрономічна обсерваторія НАН України Кинематика и физика небесных тел MS1: Decameter Radioastronomy Variations of the quasar radio spectra with period 130 h⁻¹ Mpc Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc |
| spellingShingle |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc Khodyachikh, M. MS1: Decameter Radioastronomy |
| title_short |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc |
| title_full |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc |
| title_fullStr |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc |
| title_full_unstemmed |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc |
| title_sort |
variations of the quasar radio spectra with period 130 h⁻¹ mpc |
| author |
Khodyachikh, M. |
| author_facet |
Khodyachikh, M. |
| topic |
MS1: Decameter Radioastronomy |
| topic_facet |
MS1: Decameter Radioastronomy |
| publishDate |
2005 |
| language |
English |
| container_title |
Кинематика и физика небесных тел |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
It is known that the spatial distribution of galaxies and quasars is structured at a scale LS = 130 h⁻¹Mpc. The same scale can be present at a spatial distribution of the physical characteristics of quasars. The search of period ≈ LS was conducted in the radiospectral indices of quasars in a centimetre range. The Veron-Cetti & Veron catalogue [10] was used as source. In the power spectra of series of spectral indices and proper distances of quasars the peak corresponding to the expected period confidently emerges. 0.23 ± 0.03 estimation of the parameter of density was obtained by the method of smoothing the period in different ranges of z at the varying parameter of density in the flat model of Universe. Interpretation of argument of periodicity, as proper distance, results in a geocentrism. The conformable time is proportional to proper distance and is also a good approximation of the argument of periodicity when the parameter of density equals to 0.23. At the temporal character of the exposed periodicity the centred position of the observer is not required. In such interpretation the exact expression for the argument of periodicity is unknown. The proper distance or the conformable time is introduced by its true values with an accuracy not worse than 1%.
|
| issn |
0233-7665 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/79606 |
| citation_txt |
Variations of the quasar radio spectra with period 130 h⁻¹ Mpc / M. Khodyachikh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 71-74. — Бібліогр.: 10 назв. — англ. |
| work_keys_str_mv |
AT khodyachikhm variationsofthequasarradiospectrawithperiod130h1mpc |
| first_indexed |
2025-12-07T15:49:24Z |
| last_indexed |
2025-12-07T15:49:24Z |
| _version_ |
1850865157948833792 |