Astronet Ïîèñê ïî àñòðîíîìè÷åñêèì ñàéòàì English Russian
       
        Òî÷íàÿ ôîðìà ñëîâ   Î ïðîåêòå   Ñàéòû   Ñïðàâêà
Ïîèñê ïî:www.sao.ru/    - Ïîèñêàòü ïî âñåì ñåðâåðàì
Íàéäåíî äîêóìåíòîâ: 2853 ---- Âðåìÿ ïîèñêà: 3.63ñåê.   
Êàòàëîã àñòðîíîìè÷åñêèõ ðåñóðñîâ

  • Íàáëþäåíèÿ, èíñòðóìåíòû è áàçû äàííûõ
  • Àñòðîìåòðèÿ è ñëóæáà âðåìåíè
  • Íåáåñíàÿ ìåõàíèêà è ãðàâèìåòðèÿ
  • Òåîðåòè÷åñêàÿ àñòðîôèçèêà
  • Ñîëíå÷íàÿ ñèñòåìà
    		•
  • Çâåçäû
  • Ãàëàêòèêè, êâàçàðû, êîñìîëîãèÿ
  • Èññëåäîâàíèå êîñìîñà
  • Îáùèå âîïðîñû
  • Ïðî÷åå

    • [ Â íà÷àëî ] Ïðåä. | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | Ñëåä.

    91. 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
    Ïîõîæèå äîêóìåíòû

    92. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_392_131W.pdf
    ... 2.12 2.17 2.19 2.17 2.20 2.12 2.09 2.09 [µm] 0.28 0.14 0.31 0.32 0.02 0.33 0.41 0.33 ... indicates the optical depth at 2.2 µm (measured from the star), that would build up ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_392_131W.pdf -- 681.5 Êá -- 24.02.2010
    Ïîõîæèå äîêóìåíòû

    93. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2008/aj_135_5_1803.pdf
    ... 00475 ± 0. 0005 and reasonable masses for its components of 2.1 M and 2.0 M , in good agreement with standard calibration (Gray ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2008/aj_135_5_1803.pdf -- 173.8 Êá -- 24.02.2010
    Ïîõîæèå äîêóìåíòû

    94. Handbook of RATAN-600 Continuum observer
    ... 20h42m54.855s V(car)/V(src) 0.00 Start time 18h30m58.88s Time before RA m 2.500 Stop time 18h35m28.88s Time after RA m 2.000 ... Òðóøêèí) . A_eff( 2.7cm) = 3.072*H + 360.5 m 2 ( 4 o - 80 o ) . A_eff( 7.6cm) = 4.653*H + 574.4 m 2 (20 o - 80 o ) . ...
    [ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/hq/lran/manuals/index.html.ru -- 98.2 Êá -- 01.10.2012
    Ïîõîæèå äîêóìåíòû

    95. Êðàòêèå ñâåäåíèÿ î Ñîëíöå
    ... http://www.ovro.caltech.edu/ . OVRO, . 27 x 2 m 5 x 2 m . http://www.nro.nao.ac.jp . ...
    [ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/hq/sun/edu/radioastr_rus.html -- 15.5 Êá -- 01.10.2012
    Ïîõîæèå äîêóìåíòû

    96. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p435.pdf
    ... stars were obtained with the CORALIE spectrograph at the 1.2­m Euler telescope in La Silla during a programme, dedicated to the ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p435.pdf -- 244.7 Êá -- 11.08.2011
    Ïîõîæèå äîêóìåíòû

    97. http://www.sao.ru/cats/~satr/RFSymp/abs/15_Hovatta.ps
    ... LONG­TERM RADIO TIME SCALES OF ACTIVE GALACTIC NUCLEI T. Hovatta 1 , M. Tornikoski 1 , M. Lainela 2 , E. Valtaoja 2 , I. Torniainen 1 , M.F. Aller 3 , H.D. Aller 3 1 Mets˜ahovi radio Observatory Mets˜ahovintie 114 02540 Kylm˜al˜a, Finland 2 Tuorla ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/cats/~satr/RFSymp/abs/15_Hovatta.ps -- 67.1 Êá -- 09.10.2006
    Ïîõîæèå äîêóìåíòû

    98. Cosmology Tutorial - Part 4
    ... For the largest elementary particle mass usually considered, the Planck mass M defined by 2*pi*G*M 2 = h*c, this density is 2E91 gm/cc. ...
    [ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/cats/~satr/cosmo/cosmo_04.htm -- 12.2 Êá -- 16.10.2000
    Ïîõîæèå äîêóìåíòû

    99. A Catalogue of Linear Polarization by Tabara Inoue
    ... z.zzzz S_6/Jy RM/rad/m^2 IPA +- G Pm/% DP/cm Notes ----+----1----+----2----+----3 ... Column 13:radio flux densities in Jy (= 10^26 W/Hz/m^2) at 6 cm. ... of RM search was less than 200 rad/m^2 except at low galactic latitudes (cot |b| < 2 ...
    [ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/cats/doc/POL_Tabara.html -- 24.0 Êá -- 18.03.2015
    Ïîõîæèå äîêóìåíòû

    100. http://www.sao.ru/cats/~satr/RFSymp/abs/15_Hovatta.pdf
    ... LONG-TERM RADIO TIME SCALES OF ACTIVE GALACTIC NUCLEI T. Hovatta 1 , M. Tornikoski 1 , M. Lainela 2 , E. Valtao ja 2 , I. Torniainen 1 , M.F. Aller 3 , H.D. Aller 3 Mets¨ vi radio Observatory aho Mets¨ vintie 114 02540 Kylm¨ a, Finland aho al¨ Tuorla ...
    [ Òåêñò ]  Ññûëêè http://www.sao.ru/cats/~satr/RFSymp/abs/15_Hovatta.pdf -- 23.6 Êá -- 09.10.2006
    Ïîõîæèå äîêóìåíòû

    [ Â íà÷àëî ] Ïðåä. | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | Ñëåä.

    Rambler's Top100 RFBR ßíäåêñ öèòèðîâàíèÿ