Cyclical accretion regime change in the slow X-ray pulsar 4U 0114+65 observed with Chandra

Graciela Sanjurjo-Ferrín, Jose Miguel Torrejón, Konstantin Postnov +5

4U 0114+65 is a high-mass X-ray binary system formed by the luminous supergiant B1Ia, known as V{*} V662 Cas, and one of the slowest rotating neutron stars (NS) with a spin period…