Pulse profiles of millisecond pulsars and their Fourier amplitudes

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dc.creatorPoutanen, Juri
dc.creatorBeloborodov, Andrei M.
dc.date2006-08-30
dc.date2006-11-23
dc.date.accessioned2026-07-07T10:23:31Z
dc.date.available2026-07-07T10:23:31Z
dc.descriptionApproximate analytical formulae are derived for the pulse profile produced by small hot spots on a rapidly rotating neutron star. Its Fourier amplitudes and phases are calculated. The proposed formalism takes into account gravitational bending of light, Doppler effect, anisotropy of emission, and time delays. Its accuracy is checked with exact numerical calculations.
dc.description9 pages, 6 figures; replaced with the version published in MNRAS
dc.identifierhttps://arxiv.org/abs/astro-ph/0608663
dc.identifierhttp://arxiv.org/abs/astro-ph/0608663
dc.identifierMon.Not.Roy.Astron.Soc.373:836-844,2006
dc.identifierdoi:10.1111/j.1365-2966.2006.11088.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175859
dc.subjectAstrophysics
dc.titlePulse profiles of millisecond pulsars and their Fourier amplitudes
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