... of lambda Ori A, delat Ori A, alpha Cam, 19 Cep, iota Her, rho Leo and other stars were obtained with using 1-m and 6-meter telescope of Special Astrophysical Obser- vatory and 1.8-m telescope of Bohinsan Astronomical Observatory (Korea) were obtained ...
... 2.22 · 10-7 e3 Sli , (1.2) Thus, the transition probabilities can b e expressed by oscillator strengths in the form gl AE li 1,M 1 = 8.01 · 109 e2 gi fil , gl AE 2 = 8.02 · 109 e2 gi fil , li (1.3) Taking into account the conservation laws of momentum ...
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Ссылки http://www.astro.spbu.ru/staff/afk/AtDatCentre/AtDatCat/Chapter1.pdf -- 64.7 Кб -- 19.11.2010 Похожие документы
... The improvement in the quality of spectral observations associated with the launch of the Hubble telescope and the operation of large telescopes with mirror diameters of 8-10 m has led to the discovery of extreme inhomogeneity in planetary nebulae. ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2008/Kholtygin2008NeTediagnE.pdf -- 157.1 Кб -- 19.11.2010 Похожие документы
... 8 ... F 2 (see Eq. (8)) by the replacement of m ij for m ji , where m ij = m i =m j . ... m quartz = 1:5 0:0077i and m carbon = 2:8 0:533i. The intensity distribution inside ...
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Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS/P4-MINSK/PUBL/TEXT/avw-ao.ps -- 175.6 Кб -- 19.11.2010 Похожие документы
... of the de Vaucouleurs law is lg or, in units of m / I (r ) = -3.33071 Ie 1/4 r re -1 , , µ(r ) = µe + 8.32678[(r /re )1/4 - 1 ... M( r ) = M0 (8.58, r 1/4 j (r )rdr r 2 -R . ...
... b that ( )( ) 0 1 1 3 w - - = g k , (10) ( ) g k m - = 1 3 8 , (11) ( ) g k s - - = 1 3 4 1 a , (12) ( ) ( ) ( ) ( ) ( ) 0 0 0 ... A2.1. One can see that the accuracy is high. The error is smaller than 7% up to m Е l 8 . 1 = . ...
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Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS/P4-MINSK/PUBL/TEXT/k-irs.ps -- 293.0 Кб -- 19.11.2010 Похожие документы