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    • [ Â íà÷àëî ] Ïðåä. | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | Ñëåä.

    71. http://www.sao.ru/hq/marat/publ/articles/Afanasev_engl.pdf
    ... range ° ° 3600­10000 A, the 2.1-m Cananea telescope (Mexico) in the range 4200­9000 ... are classified by using the 2.1-m G. Haro Observatory (GHAO) telescope of the ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/marat/publ/articles/Afanasev_engl.pdf -- 405.5 Êá -- 24.02.2010
    Ïîõîæèå äîêóìåíòû

    72. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p061.pdf
    ... is determined by the expression (Gnedin & Silant'ev, 1997): = 0.4 1µm 2 B 1 cos = cos , 1G 2 (1) where is the wavelength of ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p061.pdf -- 374.0 Êá -- 11.08.2011
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    73. 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 ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/cats/~satr/RFSymp/abs/26_Nieppola.ps -- 86.8 Êá -- 09.10.2006
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    74. Physical Constants and Astronomical Data
    ... Astronomical unit AU 1.496 13 cm Parsec pc 3.086 18 cm Light year ly 9.463 17 cm Solar mass M o 1.99 33 g Solar radius R o 6.96 10 cm Solar luminosity L o 3.9 33 erg s -1 Solar Temperature T o 5.780 3 K ...
    [ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/drabek/CONSTANTS/2/constants.html -- 8.1 Êá -- 13.01.2000
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    75. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2008/aj_135_5_1803.pdf
    ... performed several runs with the 1.52 m telescope of the Observato´ ´ rio Astronomico ... Systemic mass (M ) 1 2 3 4 3 2 2 3 .8 .6 .1 .1 .0 .9 .8 .0 ± ± ± ± ± ± ± ± 0 1 0 0 0 ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2008/aj_135_5_1803.pdf -- 173.8 Êá -- 24.02.2010
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    76. http://www.sao.ru/drabek/CCDP/ti/datashits/socs055a.pdf
    ... 680- â 500-PIXEL CCD IMAGE SENSOR SOCS055A ­ JUNE 1996 ­ REVISED APRIL 1997 7.4 µm Clocked Barrier 3.8 µm Clocked Well Virtual Barrier 3.6 µm Antiblooming Device Virtual Well Channel Stops Including Metal Bus Lines 1.6 µm 1.6 µm Clocked Gate Figure 1 ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/drabek/CCDP/ti/datashits/socs055a.pdf -- 219.9 Êá -- 28.04.1999
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    77. http://www.sao.ru/cats/~satr/RFSymp/abs/22_Lahteenmaki.ps
    ... PLANCK --- UNLOCKING THE SECRETS OF THE UNIVERSE A. L˜ahteenm˜aki 1 , M. Tornikoski 1 , J. Aatrokoski 1 , E. Valtaoja 2 1 Mets˜ahovi Radio Observatory, Helsinki University of Technology Mets˜ahovintie 114, 02540 Kylm˜al˜a, Finland alien@kurp.tkk.fi 2 ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/cats/~satr/RFSymp/abs/22_Lahteenmaki.ps -- 59.7 Êá -- 09.10.2006
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    78. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2300169.pdf
    ... J images and in the 0.79 µm and 1.06 µm HST images suggest that the core of A is not ... a strong mass loss at a rate of M 2 - 5 â 10-5 M yr-1 (see e.g. Loup et al ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2300169.pdf -- 815.3 Êá -- 24.02.2010
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    79. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_529H.pdf
    ... Extensive radiative transfer calculations have been carried out and confronted with the observations taking into account the spectral energy distribution ranging from 1 µm to 1 mm, our near-infrared visibility functions at 1.24 µm, 1.65 µm and 2.12 µm, as ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_529H.pdf -- 322.5 Êá -- 24.02.2010
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    80. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2006/balega_etal_aua_hipparcosbinaries2_2006.pdf
    ... Binaries with m 1 are plotted as filled circles, while those with m > 1 are plotted as stars. ... 2004). The pairs with small magnitude differences are marked by filled circles, and those with m > 1 mag are plotted as stars. ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2006/balega_etal_aua_hipparcosbinaries2_2006.pdf -- 386.6 Êá -- 24.02.2010
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    [ Â íà÷àëî ] Ïðåä. | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | Ñëåä.

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