Long Term Timing Observations of PSR B1509-58

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dc.creatorLivingstone, Margaret A.
dc.creatorKaspi, Victoria M.
dc.creatorManchester, Richard N.
dc.date2004-02-08
dc.date.accessioned2026-07-07T02:12:10Z
dc.date.available2026-07-07T02:12:10Z
dc.descriptionWe present an updated phase-coherent timing solution for the young, energetic pulsar PSR B1509-58 for twenty years of data. Using a partially phase-coherent timing analysis, we show that the second frequency derivative is changing in time implying a third frequency derivative of (-9+/-1)x10^-32 s^(-4). This value is consistent with the simple power law model of pulsar rotation.
dc.description2 pages. To appear in "Young Neutron Stars and Their Environments"(IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B.M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0402181
dc.identifierhttp://arxiv.org/abs/astro-ph/0402181
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7364
dc.subjectAstrophysics
dc.titleLong Term Timing Observations of PSR B1509-58
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