A Possible Origin of kHZ QPOs in Low-Mass X-ray Binaries

25 Feb 2020 Kato Shoji Machida Mami

A possible origin of kHz QPOs in low-mass X-ray binaries is proposed. Recent numerical MHD simulations of accretion disks with turbulent magnetic fields of MRI definitely show the presence of two-armed spiral structure in quasi-steady state of accretion disks... (read more)

PDF Abstract
No code implementations yet. Submit your code now

Categories


  • HIGH ENERGY ASTROPHYSICAL PHENOMENA