¤ё Bа Iд Bе B¶ B» ¤ѕ sж 0а m vg u tg s gr i q l po n g m l k j gg i hg f 3 #A 9A 0X bX 2T )6 i 0C oГ 0A YC % 9 0YC h #7 26 4 94 9X DC Bt A WC f4 B$ 9A X gd 2T Y6 2X A f( e Ґ¤ 4 T S )( #4 ёў e` r( eC rr3 YX ¤ъ 4к x( 5d A ... ) % )$ B A f7 #A 0C b6 BA A Q @C hA Ґd b( #A 2 2 ' Y$ G4 Y6 4 'A $ 'd e 9( )( x §к b4 0A ( A 9aC %6 ! ... Te2 )0 )0 $a 10 h% 43 5% V T2 $# BP 5' )P ЎS V P TA "W EW )! ... 6 5 $ 50 )3 4 Ґ% ED )0 )P " Ґ Ґ§ d56 $f " T42 )% 4A 42 )% $ "f T2 $# ! ...
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Ссылки http://www.sao.ru/Doc-k8/Science/Public/Bulletin/Vol60-61/p011.pdf -- 553.0 Кб -- 25.12.2008 Похожие документы
Special Astrophysical Observatory, Nizhnij Arkhyz, 369167 Russia pea@sao.ru Magnitude Magnitude Differences measurements for speckle Differences measurements for speckle Inter ferometric binaries binaries Inter ferometric E. A. Pluzhnik A method of magnitude differences measurements for speckle interferometric binary stars is presented. The method is based on standard power spectrum analysis of speckle series without correction speckle interferometric transfer function. ...