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21. http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf
... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf -- 100.3 Кб -- 21.05.2007
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22. Postdoctoral Research Assistant
Armagh Observatory . ... Email Submission Address: lfy arm.ac.uk . ... The closing date for receipt of applications: 30/06/2008 . ... Applications are invited for a 3 year postdoctoral fellowship in Atomic Physics to be held at Armagh Observatory beginning October 2008 or as soon as possible thereafter. ... Further information about Armagh Observatory, and in particular the current research programme, may be obtained by consulting the Observatory's web-site or via email to Gerry Doyle (jgd arm.ac.uk). ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/jobs/2008/jgd-atomic.html -- 5.6 Кб -- 02.06.2008
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23. http://www.iki.rssi.ru/galeev/astro2007/barkov2007.pdf
... Models of central engines (1) Potential of disk accretion onto stellar mass black holes: disk binding energy: thin disk life time: - accreted mass - disk outer radius - gravitational radius - Shakura­Sunyaev parameter Ultra-dense Hyper-Eddington neutrino cooled disks !! ... 1989); Neutron star + Neutron star Neutron star + Black hole White dwarf + Black hole Black hole + compact disk Burst duration: 0.1s ­ 1.0s Released binding energy: (1.2) Collapsars­ origin of long duration GRBs? ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/galeev/astro2007/barkov2007.pdf -- 2039.4 Кб -- 27.02.2008
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24. Modelling Spectro-photometric Characteristics of Eclipsing Binaries
... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/polubekg.html -- 15.8 Кб -- 12.06.2006
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/polubekg.html -- 15.8 Кб -- 15.05.1998
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25. Letter to the Deputy Head of the Administration of Russian Federation President
To the Deputy Head of the Administration of Russian Federation President Mr. A.V.Ogarev . ... First the international space station (ISS) Alpha, which is under construction now, will compare to the OS Mir on the amount of information only in 5-7 years. ... Thirdly, the participation of Russian Federation in the international space projects, including work on the international space station (ISS) Alpha, is to be aimed first of all at the providing of Russian interests. ...
[ Сохраненная копия ]  Ссылки http://www.cosmoworld.ru/mirstation/english/documents/ran_211098.shtml -- 8.7 Кб -- 09.04.2016
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26. http://zebu.uoregon.edu/~uochep/talks/talks04/S2S3GR~2.pdf
Isabel Leonor University of Oregon search for short-duration GW bursts coincident with gamma-ray burst triggers ~1 to 10 ms, e.g. supernova core-collapse models, end of inspiral merger take advantage of readily-available and readilyaccessible ... triggers are from Interplanetary Network (IPN) (KonusWind, Ulysses, Mars Odyssey, others), INTEGRAL , HETE prepare for Swift triggers November 5, 2004 MIT Burst F2F Meeting I ... November 5, 2004 MIT Burst F2F Meeting I. Leonor 14 ! ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks04/S2S3GR~2.pdf -- 1629.6 Кб -- 07.02.2005
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27. Researches of Astronomy and Space Physics Department
Nowadays at the Department the experimental and theoretical investigations, including astronomical and ionospheric observations, active experiments with space vehicles are taking place. ... Solar Corona physics and erruptive phenomenae. ... Stellar astronomy. ... The Department has organized and put into practice more then 50 expeditions for observation of Solar ecllipces, aurorae polaris, comets, meteor streams, controlled space experiments, and also for investigations of geophysical characteristics. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/research.html -- 16.2 Кб -- 16.02.2005
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28. Astrophysical Research Consortium - Apache Point Observatory
... Oke (AJ, 99, 1621, 1990) has provided absolute spectral energy distributions covering the wavelength range 3200 to 9200A in AB magnitudes for 25 stars. ... The reduced magnitudes are tabulated at 1A intervals from 3300 to 4700A and at 2A intervals from 4700 to 9200A. Comparison of the fluxes with those determined elsewhere showed that Oke's absolute magnitudes are systematically brighter by 0.04 mag. The magnitudes and fluxes plotted have been corrected for this effect. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/General_Information/Standards/Spect-Phot-Standards/okestandards.html -- 7.8 Кб -- 09.05.2008
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29. Galaxy sector, archive 1997
... 1997: . The character of internal motions of gas in 7200 HI clouds in the outer region of our Galaxy was investigated according to the data of the HI survey with the RATAN-600. It turned out that the effect of turbulence, as the main mechanism of gas motion is not essential, while it was discovered that 36% of the clouds are rotating. ... Periodic variations of optical emission of the gamma, X-ray and radio pulsar GEMINGA were for the first time discovered from the observations with the BTA. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_galaxy/res1997.html -- 7.5 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/Science/results/ar_galaxy/res1997.html -- 7.5 Кб -- 10.04.2016
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30. Laboratory of materials for electrochemical technologies ISSP RAS
Chemical synthesis . ... Processing of ceramic materials, electrode systems and electrochemical cells . Synthesis of solid oxide materials for high-temperature electrochemical applications . ... X-Ray photoelectron spectroscopy (XPS), also called as electron spectroscopy for chemical analysis (ESCA), provides the information on the chemical and elemental composition of the materials. ... The kinetic energy of the electrons emitted is governed by the electron structure of the element. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lmet/en/methods/xps -- 7.3 Кб -- 10.04.2016
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31. Precisely measuring velocity of a supernova shock wave | Astronomy.com
... Tonight's Sky . ... Astronomy for Kids . ... Sky Guide . ... Precisely measuring velocity of a supernova shock wave . A research team has succeeded in measuring the expansion velocity of a shock wave of the supernova remnant W44. ... Illustration of propagation W44 shock waves in the molecular cloud. ... A research team led by Tomoro Sashida and Tomoharu Oka of Keio University in Tokyo, Japan, has succeeded in precisely measuring the expansion velocity of a shock wave of the supernova remnant W44. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2013/08/precisely-measuring-velocity-of-a-supernova-shock-wave -- 70.7 Кб -- 10.04.2016
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32. HISA Poster for the 197th Meeting of the AAS, January, 2001
... We are using Canadian Galactic Plane Survey l 74.2њ, -3.6њ < b This poster gives preliminary results for a full-fledged analysis of the gas properties and distribution of HISA features in the CGPS. ... where T ON and T OFF are observed brightnesses on and off the HISA feature, T S is the spin or excitation temperature of the HISA gas, tau is its optical depth, T C is the continuum intensity, and p is the fraction of H I emission lying behind the HISA feature. ... GIF | ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/hisa/poster/2001/ -- 13.7 Кб -- 20.11.2005
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33. Galaxy Cluster Magnifies Distant Supernova
... Explanation: How do you calibrate a huge gravitational lens? In this case the lens is the galaxy cluster Abell 383 , a massive conglomeration of galaxies, hot gas, and dark matter that lies about 2.5 billion light years away ( redshift z=0.187). ... This technique compl e ments other measures including computing the dark matter needed to contain internal galaxy motions , to confine cluster hot gas , and to create the gravitational lens image distortions. ... The Hercules Cluster of Galaxies . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1310159 -- 16.6 Кб -- 05.05.2014
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34. http://www.astro.spbu.ru/staff/ilin2/INTAS2/DOCS/summary.txt
PROJECT SUMMARY (max 3000 characters) The principal goals of the project are the observational and theoretical investigation of complex cosmic objects where the processes of dust scattering, absorption and emission play significant roles. ... Development of light scattering theory and computer codes to calculate the optical properties of non-spherical inhomogeneous particles and laboratory measurements of light scattering characteristics of irregularly shaped particles. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS2/DOCS/summary.txt -- 4.6 Кб -- 19.11.2010
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36. IZMIRAN - Laboratory for ionosphere discontinuity investigation
... Main page . ... Main results . Data . ... webmaster@izmiran.ru . ... The main subject of the laboratory is investigation of the large-scale structure of the topside ionosphere. The researches are based on the vast bank of data of the Intercosmos-19, Cosmos-900, and Cosmos-1809 satellites. ... study of the large-scale inhomogeneous structure of the ionosphere, including the night-side and day-side main ionospheric trough, the day-side Muldrew trough, the ring ionospheric trough etc.; . ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/ionosphere/ionheterogeneity/index.shtml -- 7.9 Кб -- 09.04.2016
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37. Index of /lk/source
... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/lk/source/ -- 2.9 Кб -- 09.04.2016
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38. ASC site, Russian version
Russian . ... Very Early Universe: inflation, generation of primordial perturbations, preheating . Very Early Universe: inflation, generation of initial perturbations, preheating . Cosmic Microwave Background Radiation: anisotropy and polarization . ... Dark Energy and Dark Matter models . High Energy Astrophysics: accretion discs, cosmic rays, gamma-ray bursts . ... Astrophysics of black holes and wormholes . ...
[ Сохраненная копия ]  Ссылки http://lukash.asc.rssi.ru/_eng/sci_theme.html -- 6.1 Кб -- 31.07.2007
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39. Creating a distribution list
. A distribution list is very useful where a group of users need to communicate amongst themselves on a regular basis. Each list is given a name just like any other user. By addressing a message to the list name, the sender can be sure that everyone will receive a copy. You cannot set up a distribution list yourself. Ask your system administrator to set one up for you.
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/mail/three.6.html -- 2.0 Кб -- 17.01.1997
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40. cat5
. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.
[ Сохраненная копия ]  Ссылки http://www.wdcb.ru/stp/cat5MOD.html -- 2.2 Кб -- 18.01.2010
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