The torque reversals of 4U 1626–67
نویسندگان
چکیده
We investigated the detailed torque-reversal behavior of 4U 1626–67 in framework recently developed comprehensive model inner disk radius and torque calculations for neutron stars accreting from geometrically thin disks. The can reproduce relation between X-ray luminosity across reversals . Our results imply that: (1) rotational equilibrium is reached when equals co-rotation radius, r co , while conventional Alfvén greater than but close to ; (2) both spin-up spin-down torques are operating on either side reversal; (3) with increasing accretion rate, associated onto star gradually dominates exerted by disk. natural outcome transitions well-defined weak-propeller phases a stable,
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ژورنال
عنوان ژورنال: Astronomy and Astrophysics
سال: 2022
ISSN: ['0004-6361', '1432-0746']
DOI: https://doi.org/10.1051/0004-6361/202141772