Author(s)

Jing Wang

Institute of Astronomy and Space Science, Sun Yan-sen University, Guangzhou, China.

In accreting neutron star (NS) low-mass X-ray binaries (LMXBs), the turbulent flow in accretion disk may show magnetic structures. Its emission will vary in time due to inhomogeneous motions through and with the accretion flow. These emissions contribute to considerable X-ray variability on a wide range of timescales in all wavelengths, and down to milliseconds. In this article, we give a brief review for quasi-periodic oscillations (QPOs), one of a periodic X-ray variability, in NS/ LMXBs. Firstly, we give a brief introduction to NS/LMXBs and the fruitful QPO components. As an example, the energy dependence of normal branch oscillations in Scorpius X-1 is discussed. We mostly focus on the properties and mechanism of kilohertz QPOs—the fastest variability components that have the same order as the dynamical timescales of the innermost regions of accretion flow. Finally, we discuss the success and questions for theoretical interpretations and present the possible entry for investigation of nature of QPOs.

Accretion, Accretion Disks, Neutron Star, QPOs, X-Ray Binaries

Wang, J. (2016) A Brief Review for Quasi-Periodic Oscillations in Neutron-Star Low-Mass X-Ray Binaries. International Journal of Astronomy and Astrophysics, 6, 82-98. doi: 10.4236/ijaa.2016.61006.