论文标题
发电机磁场对积聚毫秒X射线脉冲星的观测特性的影响
Effects of dynamo magnetic fields on observational properties of Accreting Millisecond X-ray Pulsars
论文作者
论文摘要
在本文中，我们研究了毫秒的X射线脉冲星，它们是低质量X射线二进制中快速旋转的中子星。这些系统显示出磁性流动流向恒星表面时产生的连贯的X射线脉动。在这里，我们开发了积聚光盘的基本方程式，围绕在碟片内部有一个发电机产生的磁场的情况下，X射线脉冲脉冲，我们还为圆盘内部区域中的结构方程式制定了数值方法，而最高的积分率足以使光盘内部通过散射和电子偏高的跨度差异。最后，我们通过发电机磁场对积聚毫秒X射线脉冲星的影响进行了检查。
In this paper, we have investigated the accreting millisecond X-ray pulsars, which are rapidly rotating neutron stars in low-mass X-ray binaries. These systems show coherent X-ray pulsations that arise when the accretion flow is magnetically channeled to the stellar surface. Here, we have developed the fundamental equations for an accretion disc around accreting millisecond X-ray pulsars in the presence of a dynamo generated magnetic fields in the inner part of the disc and we have also formulated the numerical method for the structure equations in the inner region of the disc and the highest accretion rate is enough to make the inner region of the disc which is overpowered by radiation pressure and electron scattering. Finally, we have examined our results with the effects of dynamo magnetic fields on accreting millisecond X-ray pulsars.
