Weak microlensing effect and stability of pulsar time scale

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dc.creatorPshirkov, M. S.
dc.creatorSazhin, M. V.
dc.date2006-10-23
dc.date.accessioned2026-07-07T07:27:05Z
dc.date.available2026-07-07T07:27:05Z
dc.descriptionAn influence of the weak microlensing effect on the pulsar timing is investigated for pulsar B1937+21. Average residuals of Time of Arrival (TOA) due to the effect would be as large as 10 ns in 20 years observation span. These residuals can be much greater (up to 1 ms in 20 years span) if pulsar is located in globular cluster (or behind it).
dc.description11 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0610681
dc.identifierhttp://arxiv.org/abs/astro-ph/0610681
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117259
dc.subjectAstrophysics
dc.titleWeak microlensing effect and stability of pulsar time scale
dc.typetext

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