Timing of the accreting millisecond pulsar XTE J1814−338 |
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| Authors: | A Papitto T Di Salvo L Burderi M T Menna G Lavagetto A Riggio |
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| Institution: | Dipartimento di Fisica, Universitádegli Studi di Roma 'Tor Vergata', via della Ricerca Scientifica 1, 00133 Roma, Italy;Osservatorio Astronomico di Roma, via Frascati 33, Monteporzio Catone 00040, Italy;Dipartimento di Scienze Fisiche ed Astronomiche, Universitàdi Palermo, via Archirafi 36, Palermo 90123, Italy;Dipertimento di Fisica, Universitádegli Studi di Cagliari, SP Monserrato-Sestu, KM 0.7, Monserrato 09042, Italy |
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| Abstract: | We present a precise timing analysis of the accreting millisecond pulsar XTE J1814?338 during its 2003 outburst, observed by RXTE . A full orbital solution is given for the first time; Doppler effects induced by the motion of the source in the binary system were corrected, leading to a refined estimate of the orbital period, P orb= 15 388.7229(2) s, and of the projected semimajor axis, a sin i / c = 0.390633(9) light-second. We could then investigate the spin behaviour of the accreting compact object during the outburst. We report here a refined value of the spin frequency (ν= 314.356 108 79(1) Hz) and the first estimate of the spin frequency derivative of this source while accreting  . This spin-down behaviour arises when both the fundamental frequency and the second harmonic are taken into consideration. We discuss this in the context of the interaction between the disc and the quickly rotating magnetosphere, at accretion rates sufficiently low to allow a threading of the accretion disc in regions where the Keplerian velocity is slower than the magnetosphere velocity. We also present indications of a jitter of the pulse phases around the mean trend, which we argue results from movements of the accreting hotspots in response to variations of the accretion rate. |
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| Keywords: | stars: magnetic fields stars: neutron pulsars: general pulsars: individual: XTE J1814?338 X-rays: binaries |
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