Next: About this document Up: Old neutron star distribution Previous: References . Figure: Velocity distribution of young pulsars calculated from statistical modelling of evolution of 50,000 binary systems. ... Figure: Equal density contours for the calculated distribution of old neutron stars (in arbitrary units). Figure: Plot of (solid lines), (long-dashed lines) and (short-dashed lines) for the calculated old neutron star space distribution versus limiting distance of the sample . ...

... FOC Instrument Handbook Version 6.0 List of Figures . ... FOC Instrument Handbook . FOC Data Handbook . ... Figure 1. Diagram showing the COSTAR correction principle for the f/96 relay - 8 . ... Variation of FWHM with wavelength for the f/96 relay of the FOC - 51 . ... Figure 40. f/48 camera background as a function of time after camera switch-on - 75 . ... Table 1: Summary of FOC Performance Characteristics I. Imaging - 14 . Table 2: Summary of FOC Performance Characteristics II. ...

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... Figure eight, as double four. Figure four, as half of eight. If you skate, you would be great, . If you could make a figure eight. That's a circle that turns 'round upon itself. One times eight is two times four. Four times four is two times eight. ... One times eight is eight, two times eight is 16 . Three times eight is 24, four times eight is 32 . ... Six times eight is 48, seven times eight is 56, . ... And ten times eight is 80, that's true. ... Plus two times eight: . ...

Quiet Sun, Grevesse et al. abundances, Arnaud & Rothenflug ion balances . Figure 1: Emission Measures (EM) [cm -5 ] derived from combining all lines for particular ions, for the Active and Quiet Sun regions observed by SERTS. Error bars have been shown when multiple lines from the same ion have been combined to produce a single ion-averaged EM. ... Following Brosius et al. (1996), we have assumed solar coronal abundances derived by Feldman et al. ...

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... The OVERLAY element is used to overlay images on top of a base figure. ... UNITS . Specifies the choice of units for width and height: units=pixels (the default) specifies pixels, while units=en specifies en units (a typographical unit equal to half the point size). ... X increases to the right, and is given in pixels or en units (according to the value of the UNITS attribute). ... HEIGHT . Specifies the desired height in pixels or en units (according to the value of the UNITS attribute). ...

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. F IGURE . 7. The age distribution of the globular clusters of (a) Galactic origin and (b) accreted by the Galaxy. Different shadings are used to show the thick disk and prot-disk halo clusters. The curves are Gaussian fits to the corresponding histograms. Data was taken from ( Borkova Marsakov, 2000 ). discussion in the text | privious figure | next figure .

. Particles position in the equatorial plane, as given by our SPH simulation with gamma=1.2 after19 orbital periods. Postscript version . If you have comments or suggestions, email me at spxhmjb@astro.cf.ac.uk Last update: May 26, 1998 .

. Next: List of Tables Up: No Title Previous: Contents . Layout of the Table Editor Left Keypad . Layout of the Table Editor Right Keypad . љ . Rein Warmels . Mon Jan 22 12:06:29 MET 1996

Next: List of Tables Up: No Title Previous: Contents . Распределенная система сбора . ... Алгоритм работы сервера . ... Процесс проведения удаленных наблюдений на РАТАН-600 . ... Экспериментальная запись ошибки слежения при воздействии скачка скорости в 5 мм/с. То же при скорости 10 мм/с. То же при скорости 15 мм/с. Наблюдения источника 3С84 на волне 1.38 см. ... Разности наблюденных и предвычисленных моментов кульминации (``О - С") по наблюдениям квазаров 1148-00 и 1226+02. ...

. Figure A1. This shows the geometry of a lower support rod when weighted and unweighted by the secondary cage. From this follows the equation . which can be rewritten as . For all cases of interest we have the conditions that << 1 and << 1 so that we can effectively ignore the terms and . Doing this gives us the excellent approximation . Solving this for gives . From the figure we can also see that Z = L sin( a). Combining these last two equations gives .

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. Figure 2. The same as in figure 1 but for dependence of the FD onset (?To, panels a,b) and peak (?Tp, panels c,d) transit times on the eruptive magnetic flux ?.

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... There are two stars in the binary system: a donor star on the right and a black hole on the left (an infinitely small point in the center of a complex figure). ... The wind is ejected as a hollow cone; it has a funnel (the funnel opening angle in the figure) and thick walls (wall opening angle in the figure). The observer looks at the whole system and the supercritical disk from the right, and sees everything up to the wind photosphere (the red color in the figure). ...

. Приложение к лекции для студентов . Верходанов О.В. Рис.12. Пример работы алгоритма чистки. На верхнем рисунке приводится модельное изображение, на среднем - грязная карта, на нижнем - изображение, восстановленное с помощью CLEAN. Рисунок воспроизведен из работы Стиэра и др. (1984). vo @ sao.ru ( Oleg Verkhodanov ) .