On the torque reversals of 4U 1626--67

Abstract

We have investigated the detailed torque-reversal behavior of 4U 1626-67 in the framework of the recently developed comprehensive model of the inner disk radius and torque calculations for neutron stars accreting from geometrically thin disks. The model can reproduce the torque -X-ray luminosity relation across the torque reversals of 4U 1626-67. Our results imply that: (1) rotational equilibrium is reached when the inner disk radius equals the co-rotation radius, r co , while the conventional Alfvén radius is greater than and close to r co , (2) both spin-up and spin-down torques are operating on either side of torque reversal, (3) with increasing accretion rate the spin-up torque associated with accretion onto the star gradually dominates the spin-down torque exerted by the disk. The torque reversals are the natural outcome of transitions between the well-defined weak-propeller and spin-up phases of the star with a stable geometrically thin accretion disk.