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http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_392_937W.pdf.
http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_392_937W.pdf.
1. Origin of the internal structures in HL Tauri jet (HH 151)
... The HH flow associated with young stellar object HL Tau has an exciting history and even until now the origin of some its features is not clear yet. ... Knotty structures of Herbig-Haro jets are common phenomena and knowing the origin of such structures is essential for understanding the processes of jet formation. ... In the flow detected compact knots with high (-150 km/s) and bow shape structures in front of those, with low radial velocities (-50 km/s). ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2012/Movses/ -- 5.1 Кб -- 02.10.2012
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2. High-resolution Near-infrared Study of the Deeply Embedded Young Stellar Object
... High-resolution Near-infrared Study of the Deeply Embedded Young Stellar Object S140 IRS 3 . ... P22P We explore the structures immediately surrounding the high-mass young stellar object S140 IRS 3 within the L1204 molecular cloud. ... The S-shaped structure of this feature can be well reproduced by a model assuming a precessing outflow from IRS 3a. Furthermore, we find several elongated features pointing away from IRS 3 in a southern direction. ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/preibisch_2001.html -- 12.1 Кб -- 02.10.2012
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3. http://www.sao.ru/cats/~satr/RFSymp/abs/02_Arshakian.ps
A LINK BETWEEN VARIABLE OPTICAL CONTINUUM AND RADIO EMISSION OF A COMPACT JET IN THE RADIOнLOUD SEYFERT GALAXY 3C390.3 T.G. Arshakian 1 , A.P. Lobanov 1 , V.H. Chavushyan 2 , A.I. Shapovalova 3 , J.A. Zensus 1 , N.G. Bochkarev 4 , A.N. Burenkov 3 1 MaxнPlanckнInstitut fur Radioastronomie, Auf dem Hugel 69, 53121 Bonn, Germany, 2 Instituto Nacional de AstrofТРsica, Optica y ElectrТonica, Apartado Postal 51. ... We combine results from the monitoring of 3C390.3 in the optical region (Shapovalova et al. ...
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Ссылки http://www.sao.ru/cats/~satr/RFSymp/abs/02_Arshakian.ps -- 86.8 Кб -- 09.10.2006
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4. 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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Ссылки http://www.sao.ru/drabek/CCDP/SITe/502datsh.pdf -- 643.8 Кб -- 11.11.1998
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5. How to reach SAO
... If you have wished to reach the Special astrophysical observatory the best way is to communicate with Tatyana N.Sokolova: . SAO RAS, Nizhny Arkhyz, . ... A visit to the 6-meter optical telescope BTA, the radiotelescopes RATAN-600 of 600 m in diameter of SAO RAS and the new 32-m dish of the Institute of Applied Astronomy of RAS. ... The visit to SAO, including meals, airflight and local transportation and accommodation, will cost a total of about 220 USD per person. ... 8 USD/per person/per night . ...
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Ссылки http://www.sao.ru/hq/lran/vo/how_get_SAOe.html -- 4.9 Кб -- 01.10.2012
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