... with a probable mass of mv 2.9 M ), we concluded that mx 2.45-2.55 M (for i = 75 -90 ... high upper mass limit: 2.95 M for nonrotating and 3.45M for rotating stars [9, 10 ...
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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
... X-7 was derived from the observed radial-velocity curve in [9]: mx = 15.65 ± 1.45M ... 3.20 M and 15.65 ± 1.45M , respectively (for the most probable mass of the optical ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_M33_X7_eng.pdf -- 648.2 Кб -- 03.03.2009 Похожие документы
... by the wind model of Kudritzki and Reimers [45]: m LR/m. (8) The change of the star ... mass of the star. range 2-7 M , while about 45% of the black holes have masses of 7 ... The fraction of black holes with masses exceeding 7.5 M is also 45%. ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_BH_evolution_eng.pdf -- 210.4 Кб -- 23.06.2005 Похожие документы
... 45) M. Kaufman, S. Pasynok, Development of the methods and technics of the Russian National EOP service //Measuring equipment, 2005, N 1, P. 24-27(in Russia). ...