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 . ...

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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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. 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 .

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. 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

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. 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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