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http://hdl.handle.net/2289/3009
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DC Field | Value | Language |
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dc.contributor.author | Hari Dass, N.D. | - |
dc.contributor.author | Radhakrishnan, V. | - |
dc.date.accessioned | 2007-06-20T06:30:19Z | - |
dc.date.available | 2007-06-20T06:30:19Z | - |
dc.date.issued | 1975-02 | - |
dc.identifier.citation | Astrophysical Letters, 1975, Vol.16, p135-139. | en |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | http://hdl.handle.net/2289/3010 | - |
dc.description | Restricted Access. | en |
dc.description.abstract | The possibility of observing gravitational spin precession due to spin-orbit coupling in a binary pulsar system is considered. An analysis is presented which can aid in delineating the relevant physical effects from pulse-structure data. In this analysis, it is assumed that the pulsar radiation emanates from a cone whose axis is tilted with respect to the axis of rotation. It is found that the time-averaged pulse width and polarization sweep vary periodically with time and that this variation has a periodicity of the order of the spin-precession frequency averaged over a complete revolution. It is concluded that for an orbital period of about 180 years, it suffices to measure polarization data with an accuracy of a few parts in 100 over a period of six months to a year in order to uncover the effects of spin precession. The consistency of the analysis is checked, and the calculations are applied to a recently discovered binary pulsar. | en |
dc.format.extent | 337161 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Gordon and Breach Science Publishers. | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?1975ApL....16..135H | en |
dc.rights | 1975 Gordon and Breach Science Publishers. | en |
dc.subject | Binary stars | en |
dc.subject | Gravitational effects | en |
dc.subject | Precision | en |
dc.subject | Pulsars | en |
dc.subject | Relativistic effects | en |
dc.subject | Spin-orbit interactions | en |
dc.subject | Pulse duration | en |
dc.subject | Stellar radiation | en |
dc.title | The new binary pulsar and the observation of gravitational spin precession | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1975 Astro. Letters V16 p135.pdf Restricted Access | Restricted Access | 329.26 kB | Adobe PDF | View/Open Request a copy |
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