Search results for "X-rays: individuals: XTE J1814−338"

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Indications of non-conservative mass-transfer in AMXPs

2019

Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members. All AMXPs are transients with usually very long quiescence periods, implying that mass accretion rate in these systems is quite low and not constant. Moreover, for at least three sources, a non-conservative evolution was also proposed. Aims. Our purpose is to study the long term averaged mass-accretion rates in all the Accreting Millisecond X-ray Pulsars discovered so far, to investigate a non-conservative mass-transfer scenario. Methods. We calculated the expected mass-transfer rate under the hypothesis of a con…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsCompact star01 natural sciencesLuminositystars: neutronX-rays: binariesPulsarpulsars: general0103 physical sciencesX-rays: individuals: IGR J17498−2921X-rays: individuals: IGR J17498-2921010303 astronomy & astrophysicsX-rays: individuals: XTE J1814−338PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsX-rays: binarieX-rays: individuals: XTE J1814-338Radiation pressureSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Magnetic dipole
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