... hence, for the sought-for mixing time m (rmin ): m (rmin )v0 n r 2 min using the ... m d N. Comparison of the m values in a globular cluster (m 106 107 yr) and the ... m , a stellar system is described The latter agrees well with the result by Genkin ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/Papers/Stohastization_Time.pdf -- 489.3 Кб -- 24.12.2005 Похожие документы
... 101 100 SW UMa AM Her DQ Her tation radius and (1)(4), we obtain the minimum temperature of the accretion zone in the blackbody approximation kTmin = 0.94 M1 1/12 L R 1/4 35 3/4 6 P 1/6 kev. (5) kTmin kTspec Her X 1 Vela X 1 X0331 + 53 4U0115 + 63 ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/article1_eng.pdf -- 142.3 Кб -- 12.09.2003 Похожие документы
... Cosmic Dusty Plasmas . DA Mendis, M Rosenberg . 32:419-63 . The Kuiper Belt . ... 34:35-73 . Charged Dust Dynamics in the Solar System . M Horanyi . 34:383-418 . ... Flares on the Sun and Other Stars . В Haisch, KT Strong, M Rodono . 29:275-324 . ...
... Journal: V.31, v.101 Informations. relative to: absolute reference frame ... Minute of right ascension (alpha, m) 7. Second of right ascension (alpha, s) 8. ... N Year Day with alpha delta OBS N sat Month decimals h m s deg ' '' MPC Mag ...