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Geodetic Precession and the Binary Pulsar B1913+16

Abstract:
A change of the component separation in the profiles of the binary pulsar PSR B1913+16 has been observed for the first time (Kramer 1998) as expected by geodetic precession. In this work we extend the previous work by accounting for recent data from the Effelsberg 100-m telescope and Arecibo Observatory and testing model predictions. We demonstrate how the new information will provide additional information on the solutions of the system geometry.

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Publication date:
2000-02-04
Keywords:
Pubs id:
pubs:180682
UUID:
uuid:b625d31f-ad63-400e-a294-35913e93dff7
Local pid:
pubs:180682
Source identifiers:
180682
Deposit date:
2012-12-19

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