... This yields the first constraint on B and - M : B ! 4:6 \Delta 10 9 M5=6 1:4 R \Gamma3 6 - M 1=2 \Gamma15 G; (8) 2. ... 2 cap oeT 4 = GM - M R we find the additional relation between B and - M : B = 2:5 \Delta 10 7 (T=79 eV) 7 R 4 6 M \Gamma3=2 1 ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/html/publications/pazh/kon.ps -- 263.6 Кб -- 29.10.1997 Похожие документы
... 5 1/20 7 1/10 R (18) h , R -3/5 7 2 = 5.1 в 10 m в f (R)3/5 0.6 3/5 M17 - T T T T 1 ... 1 - 4 and f (R) = 1): R BC 0 0.10 B C 5 в 107 m в 0 0 1/3 2/3 M17 T T 0.6 -1/3 -2/3 ...
... grd , and monitoring each iteration, try: surface hawaii_5x5.xyg -R 198/208/18/25 -I 5m -G hawaii_grd.grd -T 0.25 -C 0.1 -VL surface will complain when more than one data point is found for any node and suggest that you run blockmean , blockmedian , or ...
... B =200 pc MB = 8:07 \Delta 10 10 M fi Halo d 0 =277 pc M 0 = 5:0 \Delta 10 10 M fi The density in our model is constant in time ... NNS = 10 9 S.B. Popov & M.E. Prokhorov: Spatial distribution of the accretion luminosity 5 Fig. 4. ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/html/publications/aa/foraa1.ps -- 239.0 Кб -- 23.10.1997 Похожие документы
... This yields the first constraint on B and — M : B ! 4:6 \Delta 10 9 M5=6 1:4 R \Gamma3 6 — M 1=2 \Gamma15 G; (2) 2. ... polar caps is radiated away we find the additional relation between B and — M : B = 2:5 \Delta 10 7 (T=79 eV) 7 R 4 6 M \Gamma3 ...
[
Текст
]
Ссылки http://xray.sai.msu.ru/~polar/html/publications/snegiri/snegiri.ps -- 99.7 Кб -- 19.07.1999 Похожие документы
... 277 pc&$M_D=1.12\cdot 10^{10} M_{\odot}$\\ Bulge&$a_B$=3.7 kpc&$b_B$=200 pc&$M_B=8.07\cdot 10^{10} M_{\odot}$\\ Halo & &$d_0$=277 pc&$M_0=5.0 \cdot 10^{10} M_{\odot}$\\ \end{tabular} %\end{table*} \vskip 0.1cm The density in our model was constant in time ...