期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 375, 期 3, 页码 971-976出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2006.11359.x
关键词
stars : magnetic fields; stars : neutron; pulsars : general; pulsars : individual : XTE J1814-338; X-rays : binaries
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 (nu = 314.356 108 79(1) Hz) and the first estimate of the spin frequency derivative of this source while accreting [nu = (-6.7 +/- 0.7) x 10(-14) Hz s(-1)]. 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.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据