... D [g -2/5 cm 28/5 s -17/5 ] = 2.42в10 38 # 4/5 m 6/5 x # µ 0.5 # -4/5 # # 4 3 # 4 # -1/5 expression (29): Z o r = 0.04 # -1/2m -1/4 x # r r out # -1/20 f 1/5 # r out R# # 3/4 # t 10 d # -1/2 (# 1 # 3 ) 1/2 expression (31): D [g -3/10 cm 5 s -16/5 ] = 5 ...
... Например, звезда 2-й звездной величины ($2^m$) в 2,512 разаярче звезды 3-й величины ($3^m$) и в 2,512 х 2,512 = 6,310 раза ... У звездКовша Б. Медведицы блеск около $2^m$, у Веги около $0^m$, а у Сириусаоколо $-1,5^m$ (его блеск в 4 раза больше, чем у ...
... V.M.Lipunov $^{1,2}$ and S.B.Popov $^{1}$\\ $^{1}$ Department of Physics, Moscow ... begin{equation} {D}=4.38\cdot 10^{-23}\dot{M} _{16}^2\eta ^2T_4\mu ^{-1}v_8^{-7} I ...
... the form [8] ds 2 = c 2 (dt 2 1 + dt 22 + ... + dt 2m ) - a 2 (t)[dr 2 + ” # 2 (r) d# 2 (n) ] where the radial coordinate in ... It is interesting that the solution is the same for all k: a = # C t 2-m , m #= 2; C ln t, m = 2. ...
... AND THE SPINDOWN THEOREM. } \vskip 0.5cm V.M.Lipunov $^{1,2}$ and S.B.Popov $^{1}$\\ $^{1}$ Department of Physics, Moscow ... by Davis $\&$ Pringle (1981) as: \begin{equation} y=\frac{\dot M}{\mu^2} \end{equation} \vskip 0.1cm There are four possible ...