Íàéäåíî äîêóìåíòîâ: 3198 (5 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.11ñåê. |
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http://www.sao.ru/cats/~satr/RFSymp/abs/program_abstracts.ps.
http://www.sao.ru/cats/~satr/RFSymp/abs/program_abstracts.ps.
1. Detection of unique bright radio flare of X-ray binary
... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...
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Ññûëêè http://www.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Êá -- 10.04.2016
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1408) - mavr.sao.ru/ )
2. Laboratory of spectroscopy and photometry of extragalactic objects : Vortex
... Galaxies which were observed in the project . Location of vortex centers . Laboratory simulations . ... Vortex structure of NGC 157 . Vortex structure of our Galaxy . ... Line-of-sight velocity fields of gas with high precision and resolution are planned to be obtained for the sample of galaxies with regular spiral structure to reveal systematic deviation from circular rotation and to analyze it on the base of hydrodynamical models, which are in progress. ... Back to Laboratory Home Page. ...
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Ññûëêè http://www.sao.ru/hq/lsfvo/vortex/vortex.html -- 4.8 Êá -- 01.10.2012
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3. http://www.sao.ru/cats/~satr/RFSymp/abs/26_Nieppola.ps
SPECTRAL ENERGY DISTRIBUTIONS AND 37 GHz MONITORING OF BL LACERTAE OBJECTS E. Nieppola 1 , M. Tornikoski 1 , A. L˜ahteenm˜aki 1 , E. Valtaoja 2 1 Mets˜ahovi Radio Observatory Mets˜ahovintie 114, 02540 Kylm˜al˜a, Finland 2 Tuorla Observatory V˜ais˜al˜antie 20, 21500 Piikki˜o, Finland eni@kurp.hut.fi BL Lacertae objects (BL Lacs) are a group of active galactic nuclei (AGN) characterized by strong and rapid variability, strong optical polarization and a lack of prominent emission lines in their spectra. ...
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Ññûëêè http://www.sao.ru/cats/~satr/RFSymp/abs/26_Nieppola.ps -- 86.8 Êá -- 09.10.2006
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>599) - www.sao.ru/ )
4. Group for study of galaxies and cosmology, history
... In LABORATORY OF RADIO ASTROPHYSICS OF SPECIAL ASTROPHYSICAL OBSERVATORY OF RAS . ... History . ... Current problems of the group research interests: . study for cosmic microwave background, . study of radio galaxies (identification, evolution, statistical investigation of population), . investigation of the RATAN-600 antenna, . observations in the survey mode with RATAN-600 and their analysis, . creation of the software for data analysis. vo @ sao.ru ( Oleg Verkhodanov ) ...
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Ññûëêè http://www.sao.ru/hq/lran/vo/group/gr_resea_E.html -- 2.5 Êá -- 02.10.2012
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(Ïîêàçàòü âñå ðåçóëüòàòû (>3) - sed.sao.ru/ )
5. http://www.sao.ru/drabek/CCDP/SITe/502datsh.pdf
... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...
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Ññûëêè http://www.sao.ru/drabek/CCDP/SITe/502datsh.pdf -- 643.8 Êá -- 11.11.1998
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