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When the angular diameter of CP1919 was measured, it turned out to be small If it were visible, it would look like a flickering point of light This did not come as a surprise to astronomers The brevity of the pulse period and the shortness of the pulses themselves suggested a generating source that could be no more than a few hundred kilometers across What sort of star could be that small and yet emit such powerful electromagnetic (EM) bursts Scientists began to develop theories to account for the observations, but the task proved difficult Calculation of the distance to CP1919 indicated that it is about 400 light-years away This determination was made using an ingenious scheme At progressively longer wavelengths, the ticks from a pulsar arrive on Earth at greater and greater intervals That is, the period of the pulsar depends on the wavelength to which a radio-telescope receiver is tuned This takes place because the speed of EM wave propagation depends on the wavelength In a perfect vacuum, all EM waves, however long or short, propagate at the same speed, approximately 299792 108 m/s In interstellar space, however, which is not a perfect vacuum, radio waves travel slower than infrared, which in turn travels slower than visible light (The effect is not peculiar to pulsars; it occurs for ordinary stars and emission nebulae as well) This difference in propagation speed is tiny Sophisticated instruments are required to detect it This phenomenon is called dispersion, and it is the same effect that causes a prism to split white light into the colors of the rainbow

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The greater the distance to a pulsar, the more dispersion takes place, and the greater is the variation in the period as a function of wavelength Knowing the extent to which dispersion occurs as a function of the wavelength, astronomers can calculate the distance to almost any pulsar because the pulse intervals are as regular as the output of an atomic clock It is as if these objects were made-to-order distance-measurement devices

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implement the best practices of the Database Machine and of the Oracle Database 11g Release 2 Although implementing best practices is not a requirement, the process is generally well worth the effort, as it can fully unlock the potential of the Database Machine environment and to get the extra improvements in performance Estimating the costs of refactoring will depend on the lines of code (LOC) or the number of objects considered for refactoring, along with the complexity of the changes Generally, the higher the LOC and degree of complexity of the code, the more resource consuming and complex the refactoring will be When moving from non-Oracle systems, refactoring of the database schema can be performed using automated tools, which will be discussed in the migration steps Refactoring of other objects will be mostly manual, and the tools will be of little or no help

The better way is to click on Website Add New Item , then add a normal Web Form. Call the new page Home.aspx, and be sure to check both the Select master page and Place code in separate file checkboxes, as indicated in Figure 6-8. When you click the Add button, the Select a Master Page dialog will open. Choose CorpMasterPage.master (the only master page available at this point), and click OK. Switch to Design view. Your new Home.aspx page will be shown within the master page. The Content box will allow you to add any content you like, including controls, text, and so forth, but the contents of the master page will be inaccessible. Add some text and format it as HTML Heading 1 using the Block Format drop-down menu, as indicated in Figure 6-9. The Design view allows you to see how your new page will look when it is combined with the master page at runtime.

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