AbstractThe double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.
Changes in radio emission from PSR J0737–3039B
Advances in Space Research ; 38 , 12 ; 2725-2727
2005-11-16
3 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Changes in radio emission from PSR J0737-3039B
British Library Conference Proceedings | 2006
|Changes in radio emission from PSR J0737–3039B
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|The double-pulsar binary J0737–3039
Online Contents | 2006
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Elsevier | 2005
|The double-pulsar binary J0737-3039
British Library Conference Proceedings | 2006
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