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21. Methods and results of radio cosmology. Results
... Introduction (in Russian) . Chapter 2 (in Russian) . ... Detection of non-Gaussianity in observational CMB data . Methods of phase-analysis for component separation and CMB restoration . New pixelization scheme for the sky CMB maps and the package GLESP to CMB study in this pixelization scheme . New estimates of cosmological parameters using ages of FRII radio galaxies . ... New methods of creation of astrophysical data bases and their implementation in the databases of CATS and SEDs . ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/~vo/disser/results_e.html -- 2.9 Кб -- 27.11.2005
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22. http://star.arm.ac.uk/~ambn/abstract179.html
We perent radio flux measurements at 5 GHz for a sample of RS CVn-type chromospherically active binary systems made from 1988 to 1992 using the NRAL broad-band interferometer (BBI). The derived radio luminosities are consistent with previous observations but show that radio flaring is a common feature which will affect the results of rotation-activity studies. ... Key words: stars: activity - stars: late type - stars: binaries: close - stars: flare - stars: variables - stars: radio continuum ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract179.html -- 1.7 Кб -- 31.05.1996
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23. Raquel Salmeron - Research Interests and Experience
My research interests are focussed on the theory and modelling of accretion processes as well as star and planet formation mechanisms. I am particularly interested in the stability properties of accretion discs, the generation of MHD turbulence and associated angular momentum transport, disk - planet interactions and the origin and characteristics of jets and winds from accreting systems . ... These results have been published in Salmeron & Wardle, 2005, M.N.R.A.S., 361: 45-69. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~raquel/interests2.html -- 7.8 Кб -- 01.10.2012
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24. Application of the Minimum Determination Algorithm to the Study of the Fine
... The available observational data on masses and/or luminosities of binary components and the current models for different chemical compositions of Pop I stars were used to improve the mass-luminosity relation for stars of moderate masses. ... This technique was also applied to decompose the low-mass components of several stars suspected to be unresolved binaries. ... The method is based on the minimum determination technique applied to functions of several variables covering a limited range of values...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/malkovoy2/ -- 19.6 Кб -- 16.07.1999
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25. astro-ph
... arXiv.org . astro-ph . ... We fit the near-infrared to radio spectral energy distributions of 30 luminous and ultra-luminous infrared galaxies with pure starburst models or models that include both starburst and AGN components to determine important physical parameters for this population of objects. In particular we constrain the optical depth towards the luminosity source, the star formation rate, the star formation efficiency and the AGN fraction. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=-- -- 15.2 Кб -- 12.09.2010
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26. http://selena.sai.msu.ru/San/Publications/ms38/ms059.pdf
... The analysis shows, that asteroid ­ rubble pile loses its fast fragments in no time but the retaining fragments forms a compact structure immersed in dust ­ gas atmosphere, created by interaction of interplanetary medium with dispersed product of collisional evolution of asteroid. By interaction of an asteroid ­ rubble pile with interplanetary medium structures asteroid can increase its brightness on account of blowed up dust simulating phenomenon of distant comet's brightening. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/San/Publications/ms38/ms059.pdf -- 155.0 Кб -- 06.10.2008
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27. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/nmw/ -- 10.7 Кб -- 18.02.2015
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28. http://www.wdcb.ru/stp/data/ionosphere/NP-7/Readme.doc
Hourly values of parameter foF2 ( F2 layer critical frequency ) are resulted. The description of letters in the table is resulted below. DESCRIPTIVE Letters: A blanketing. ... C non-ionospheric (equipment). D above upper frequency range of equipment. E below lower frequency range of equipment. ... K particle E layer. L no sufficiently defined cusp between F layers. ... N superimposed layers. O measurement refers to o component. ... R attenuation near critical frequency. ...
[ Текст ]  Ссылки http://www.wdcb.ru/stp/data/ionosphere/NP-7/Readme.doc -- 21.5 Кб -- 18.01.2010
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29. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... ISS Russian Segment . ... Satellite Components . ... This experiment is a continuation of the "EXEC" and "SPICA" experiments conducted on-board "Mir" space station since 1992. ... A study of effects of space radiation on the last-gener