To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure firstname.lastname@example.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
Finding the population of pulsars in the Milky Way galaxy requires a knowledge of the parameters and limitations of the various surveys made with different instruments and in different regions of the sky. We list the available survey data and show how models of the galactic population can be compared with the observational data, allowing estimates of pulsar birthrate and lifetime. Determination of accurate positions of individual pulsars require a Solar System ephemeris and a complex geometrical computation. Binary pulsar orbits display reletivistic effects which can be measured with remarkable precision to yield parameters of orbits and checks on relativistic theory.
Email your librarian or administrator to recommend adding this to your organisation's collection.