Accretion disc–jet couplings in X-ray binaries
Published:
We proposed a magnetized, radiatively efficient thin accretion disc model (M-thin) to scrutinize the disc–jet couplings, and further explain the radio/X-ray correlations in the black hole/neutron star X-ray binary.
Citation: P.-X. Shen and W.-M. Gu, Monthly Notices of the Royal Astronomical Society 495, 2408 (2020).