Search results for "pulsars general"

showing 2 items of 2 documents

Timing of the accreting millisecond pulsar IGR~J17511--3057

2010

{Timing analysis of Accretion-powered Millisecond Pulsars (AMPs) is a powerful tool to probe the physics of compact objects. The recently discovered \newigrj is the 12 discovered out of the 13 AMPs known. The Rossi XTE satellite provided an extensive coverage of the 25 days-long observation of the source outburst.} {Our goal is to investigate the complex interaction between the neutron star magnetic field and the accretion disk, determining the angular momentum exchange between them. The presence of a millisecond coherent flux modulation allows us to investigate such interaction from the study of pulse arrival times. In order to separate the neutron star proper spin frequency variations fro…

Orbital elementsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)Order (ring theory)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsNeutron starSettore FIS/05 - Astronomia E AstrofisicaAmplitudeSpace and Planetary ScienceMillisecond pulsarHarmonicAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenastars neutron stars magnetic field pulsars general pulsars individual IGR J17511-3057 X-rays binaries
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Search for pulsations at high radio frequencies from accreting millisecond X-ray pulsars in quiescence

2010

It is commonly believed that millisecond radio pulsars have been spun up by transfer of matter and angular momentum from a low-mass companion during an X-ray active mass transfer phase. A subclass of low-mass X-ray binaries is that of the accreting millisecond X-ray pulsars, transient systems that show periods of X-ray quiescence during which radio emission could switch on. The aim of this work is to search for millisecond pulsations from three accreting millisecond X-ray pulsars, XTE J1751-305, XTE J1814-338, and SAX J1808.4-3658, observed during their quiescent X-ray phases at high radio frequencies (5 - 8 GHz) in order to overcome the problem of the free-free absorption due to the matter…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLuminosityInterstellar medium85-05pulsars general methods data analysis methods observational stars neutron X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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