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  Relativistic effects in the binary pulsar PSR 1913 + 16

Börner, G., Ehlers, J., & Rudolph, E. (1976). Relativistic effects in the binary pulsar PSR 1913 + 16.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5ECA-B Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5ECB-9
Genre: Proceedings

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344375.pdf (Publisher version), 225KB
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 Creators:
Börner, Gerhard, Author
Ehlers, Jürgen1, Author
Rudolph, Ekkart, Author
Affiliations:
1Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24012              

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 Abstract: The relativistic spin precession rate of a general binary system is considered. Contributions to the spin precession rate are associated with the 'magnetic type' component of the instantaneous Schwarzschild field of the second body relative to the rest frame of the moving first body, the spin-spin interaction between the two bodies, and the dragging of the inertial frame at the first body due to the translational motion of the second body. The spin precession of the binary pulsar produces changes in the observed pulse shape. The characteristics of these changes are investigated.

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 Dates: 1976
 Publication Status: Published in print
 Pages: 117-119
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 Identifiers: eDoc: 344375
Other: 1976MitAG..38..117B
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Title: Wissenschaftliche Tagung der Astronomischen Gesellschaft
Place of Event: Berlin, West Germany
Start-/End Date: 1975-09-15 - 1975-09-19

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Title: Mitteilungen der Astronomische Gesellschaft
  Alternative Title : 38
Source Genre: Journal
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