... radial-velocity curve for a 0.81M , the mass of the optical star binary, see Table ... I for mx = and with Procedure II for mx = 0.81M , mv = 1.80 M ,and i = 88 H line ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_Her_X1_eng.pdf -- 625.4 Кб -- 21.04.2008 Похожие документы
... low-mass transient X-ray binaries V404 Cyg (spectral type of the optical star K0IV) and GRS 1915+105 (spectral type of the optical star KIII) derived from rotational broadening of absorption lines are 0.7 ± 0.1 M [30] and 0.81 ± 0.53 M [31], respectively ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_2S0921_630_eng.pdf -- 228.5 Кб -- 30.05.2006 Похожие документы
... 81) M.B. Kaufman, S.L. Pasynok,Tropospheric delays from GPS and VLBI data, Book of Abstracts,Journees 2011 "Earth rotation,reference systems and celestial mechanics: Synergies of geodesy and astronomy", 19-21 September 2011,BEV Vienna, Austria,p. 32 . ...
... 81) M.B. Kaufman, S.L. Pasynok,Tropospheric delays from GPS and VLBI data, Book of Abstracts,Journees 2011 "Earth rotation,reference systems and celestial mechanics: Synergies of geodesy and astronomy", 19-21 September 2011,BEV Vienna, Austria,p. 32 . ...
... 77) and (78)н (81) for the 2 statistics, together with the numbers M of coincidences ... non-linear functions (78)н(81) for 2 M statistics, and the number of coincidences ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/Err_Estimated_Par_eng.pdf -- 972.5 Кб -- 21.01.2008 Похожие документы