Abstract
The influence of observer motion and the concomitant Doppler effect on the measured value of a pulsar period is analyzed. A method is given for computing the corrections needed for adjustment of the pulse observations to a barycentric coordinate system.
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Literature Cited
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Shabanova, T.V. (1979). Influence of the Doppler Effect in Measurements of the Periods of Pulsars. In: Basov, N.G. (eds) Techniques and Methods of Radio-Astronomic Reception / Tekhnika i Metody Radio-Astronomicheskogo Priema / Техника и Методы Радио-Астрономического Приема. The Lebedev Physics Institute Series. Springer, Boston, MA. https://doi.org/10.1007/978-1-4684-1638-1_9
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DOI: https://doi.org/10.1007/978-1-4684-1638-1_9
Publisher Name: Springer, Boston, MA
Print ISBN: 978-1-4684-1640-4
Online ISBN: 978-1-4684-1638-1
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