Accreting millisecond pulsars: one on each hand

dc.creatorLinares, Manuel
dc.creatorvan der Klis, Michiel
dc.creatorWijnands, Rudy
dc.date2006-10-30
dc.date.accessioned2026-07-07T10:40:40Z
dc.date.available2026-07-07T10:40:40Z
dc.descriptionWe report on the X-ray aperiodic timing analysis of two accreting millisecond pulsars: XTE J1807-294 and IGR J00291+5934. On the one hand, we discovered in XTE J1807-294 seven pairs of simultaneous kilohertz quasi-periodic oscillations (kHz QPOs) separated in frequency by nearly the spin frequency of the neutron star. This confirms the suspected dichotomy in the frequency separation of kHz QPOs: sometimes once and sometimes half the spin frequency. On the other hand, we found an extreme behavior in the power spectra of IGR J00291+5934: very strong variability at very low frequencies. Namely, the fractional amplitude of the variability was ~50%, the highest value found so far in a neutron star system.
dc.descriptionTo appear in the proceedings of the conference `The Multicoloured Landscape of Compact Objects and their Explosive Origins' (Cefalu, Sicily, June 2006), AIP
dc.identifierhttps://arxiv.org/abs/astro-ph/0610902
dc.identifierhttp://arxiv.org/abs/astro-ph/0610902
dc.identifierAIPConf.Proc.924:629-634,2007
dc.identifierdoi:10.1063/1.2775915
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181402
dc.subjectAstrophysics
dc.titleAccreting millisecond pulsars: one on each hand
dc.typetext

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