Speaker
张承民
Description
The kilohertz quasi-periodic oscillations (kHz QPOs) and spin frequwncies have been found in neutron stars low mass X-ray binaries (NS-LMXBs), which present the millisecond timing phenomena close to the surface of the compact objects. We summarize the following contents: (1). The correlations and distributions of twin kHz QPOs; (2). The relations of high-low frequency QPOs; (3). The QPO properties of NS Atoll and Z sources; (4). Relations between NS spins and QPOs; (5). The mechanisms of kHz QPOs; (6). The implications of kHZ QPOs, e.g., NS mass and radius, disk thickness and magnetic field of Atoll and Z source.
| Topic | X射线双星 |
|---|
Primary author
Prof.
CHENGMIN ZHANG
(NAOC)
Co-author
Prof.
DeHua WANG
(Guizhou Normal Unv)
