Modeling pulse profiles of accreting millisecond pulsars

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dc.creatorPoutanen, Juri
dc.date2008-09-14
dc.date.accessioned2026-07-07T12:04:43Z
dc.date.available2026-07-07T12:04:43Z
dc.descriptionI review the basic observational properties of accreting millisecond pulsars that are important for understanding the physics involved in formation of their pulse profiles. I then discuss main effects responsible for shaping these profiles. Some analytical results that help to understand the results of simulations are presented. Constraints on the pulsar geometry and the neutron star equation of state obtained from the analysis of the pulse profiles are discussed.
dc.descriptionInvited review, to appear in the proceedings of the workshop 'A Decade of Accreting Millisecond X-ray Pulsars' (Amsterdam, April 2008)
dc.identifierhttps://arxiv.org/abs/0809.2400
dc.identifierhttp://arxiv.org/abs/0809.2400
dc.identifierAIP Conf. proc. 1068 (2008), 77-86
dc.identifierdoi:10.1063/1.3031209
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/208184
dc.subjectAstrophysics
dc.titleModeling pulse profiles of accreting millisecond pulsars
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