fk5 ; circle ( 273.777 , -12.094 , 0.3 ) # color = green text ={95} fk5 ; circle ( 274.006 , -14.035 , 0.3 ) # color = green text ={96} fk5 ; circle ( 278.389 , - 10.569 , 0.3 ) # color = green text ={104} fk5 ; circle ( 279.505 , -6.918 , 0.3 ) # color = green text ={107} fk5 ; circle ( 280.333 , -4.941 , 0.3 ) # color = green ...

... 0.00 0.40 -1.213 Kurucz 0.000 (N) 0.000 (N) . ... 3.35 0.91 -1.737 Kurucz 0.511 (L) 0.000 (N) 0.511 8.420 -5.700 -7.740 FE1 6300.415 . ... 0.05 0.00 1.544 Kurucz 0.000 (N) 0.000 (N) . ... FE2 6302.394 . ... 0.02 0.00 -3.973 Kurucz 1.178 (L) 1.324 (L) 0.813 7.400 -4.050 -7.320 TI1 6302.846 . ... 0.02 0.00 -3.669 Kurucz 1.711 (L) 1.326 (L) 1.519 8.550 -6.520 -7.900 FE2 6369.460 40 2.8900 0 1 20.10 17.2 19.71 0.17 -4.253 Kurucz 1.996 (L) 1.860 (L) 1.860 8.460 -6.530 -7.910 TI1 6369.574 . ...

Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Projection e ects in the spectra of early-type pulsating stars P. Monta~nes Rodriguez and C.S. Je ery Armagh Observatory, College Hill, Armagh BT61 9DG, Northern Ireland. ... We have computed synthetic spectra to investigate the behaviour of p and, indeed, of the apparent line pro le for radially pulsating stars over a range of temperature and gravity with hydrogen-rich and hydrogen-poor atmospheres. ...

... This section calculates two essential details: the velocity boost needed to inject the Mars spaceship into the transfer orbit, and the arrival velocity at the orbit of Mars. ... 22c. Flight (1) . ... 24a.The Rotating Earth . ... As before, r 1 = 1 AU is the distance of Earth from the Sun, r 2 = 1.523691 AU that of Mars, and (as an approximation) both planets are assumed to move in circles. ... Lower-case v identifies velocities associated with orbits around Earth rather than around the Sun. ...

... UBV system; U,B,V photometry of A0620-00 #Ref: A A 48, 141 ( 1976 ) Duerbeck and Walter #mean errors of single brightness differences between comparison #and check star are : 0.006 (V); 0.006 (B) ; 0.009 (U) - #adopted 0.01 for all #Table: UBV magnitude differences, A0620-00 minus BD -0o1275 # = i.e. B(A0620-00) = B(comparison) + delta B # есть быстрые флуктуации яркости и цвета # по крайней мере, за полчаса (Лютый, 1976 ; Robertson, ...

Orbital Data and Parent Star Data for: OGLE-TR56 b . ... 0.000 . ... Planetary mass . ... Stellar mass . ... Stellar T_eff . Kelvin . ... Planetary T_eff . ... Stellar Radius . ... Measured Planetary Radius . ... T_circ (w/o core) . Gyr . ... T_damp (w/o core) . ... Bodenheimer, Laughlin, and Lin 2003, Astrophysical Journal, v. 592, 555-563. ... Adams and Laughlin 2006, ApJ : link . ...

... 5-GHz total flux density . ... VLBApls image at 5 GHz . color gif | contour gif | ... Correlated flux density (Jy) vs. projected baseline length plot . gif | ... flux density (Jy) . EW position (mas) . ... 0.6 0.2 . ... Other VLBI references . ... 2.3 and/or 8.4 GHz: VLBI images are available in the USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . 15 GHz: multiple epoch VLBI images are available in the VLBA 2-cm survey (Kellermann et al. ...

... Вернуться к предыдущей главе . ... ГЛАВА 18. ... В этой главе мы рассмотрим два из них: спин-орбитальное взаимодействие и увеличение массы движущегося электрона. Для учета первого процесса необходимо ввести понятие внутреннего магнитного момента электрона, тесно связанного с его собственным механическим моментом, или спином . ... Важную роль в развитии атомной физики сыграли опыты Штерна и Герлаха по исследованию отклонения атомных пучков в неоднородном магнитном поле. ... Под магнитным моментом ? ...