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Astron Astrophys ; 161: 303-4, 1986.
Article in English | MEDLINE | ID: mdl-11542034

ABSTRACT

On July 7, 1984 pulsar 0656+14 was found to exhibit a larger period than expected. Using observations from a number of sources, we have attempted to explain this discrepancy. No indications of orbital motion was found. The available evidence indicates that the star has a period derivative of 54 10(-15) s s-1 rather than 1.6 10(-15) s s-1 as previously reported.


Subject(s)
Astronomy/methods , Extraterrestrial Environment , Least-Squares Analysis
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