Ali Taani Awni Khasawneh, Mohammad Mardini, Ahmad Abushattal, Mashhoor Al-Wardat
Published 2020-02-07Version 1
The study of variation of measured cyclotron lines is of fundamental importance to understand the physics of the accretion process in magnetized neutron star systems. We investigate the magnetic field formation, evolution and distribution for several High- Mass X-ray Binaries (HMXBs). We focus our attention on the cyclotron lines that have been detected in HMXB classes in their X-ray spectra. As has been correctly pointed out, several sources show variation in cyclotron lines, this can result due to the effect of accretion dynamics, and hence that would reflect the magnetic field characteristics. Besides, the difference in time scales of variation of accretion rate and different type of companion can be used to distinguish between magnetized neutron stars.
Comments: Accepted for publication in Jordan Journal of Physic
A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines
The magnetic field strengths of accreting millisecond pulsars
Ultra-luminous X-ray sources as neutron stars propelling and accreting at super-critical rates in high-mass X-ray binaries
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