... a constant mass-to-light ratio M/L V = 3 , where the mass M and luminosity L V are ... of five clusters with R 100 kpc and log( M/M 4.5 is distinguished in Fig. 1 , but in ... The diagrams t - log( M/M ) are displayed in Fig. 2 . ...
... S.M. Grach (NIRFI, Nizhni Novgorod, Russia) . ... 8) . where . , , ? dispersion tensor, ? ... By substitution of expression (8) for spectral density of current and electric field ...
... seconds; sampling 50 complex amplitudes at 10 m sec intervals between TOAs of 228.29 ... This is design of a single 8-pulse pulse set: . ... Pulse xxxxxxxxxx #1 #2 #3 #4 #5 #6 #7 #8 xxx Units . ...
... F ig . 8. Abundance ratio [Mg/Fe] versus [Fe/H] for nearby field stars. ... Figure 8 demonstrates that field stars of different subsystems differ also in ... II, then Type Ia supernovae, and each would yield a distribution similar to Figure 8 ...
... 1989 (M/L V )=3 , где масса M и светимость L V в солнечных единицах. ... На диаграмме t-lg(M/M ) масса скоплений демонстрирует уверенный рост с возрастом. ... B., Geffert M., Colin J., Ducourant C., Odenkirchen M. & Tucholke M.-J.//Astron ...
... M. Krimski Employment CITA National Fellow 11/2004 The University of Western Ontario, London, Canada Adjunct Professor 9/2006 The University of Western Ontario, London, Canada NATO National Fellow 6/2003 6/2004 The University of Western Ontario ...
... 1996) assuming M/L V =3 Chernoff et.al. 1989 , where the mass M and luminosity L V ... In the t - log M/M ) diagram, the cluster masses clearly grow with age, with a ... B., Geffert M., Colin J., Ducourant C., Odenkirchen M. & Tucholke M.-J.//Astron ...