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A high mass X-ray binary is a binary system consisting of an accreting neutron star or black hole and an early-type star with more than 10 solar masses. A compact star produces X-ray radiation during the accretion of material from the stellar wind or Roche lobe. High-mass X-ray binaries are ideal places to study dense stars, stellar winds, material exchange between binary stars, and the evolution of massive binary stars. In this review, the observational properties, classification, and evolution of high mass X binaries are described. According to the mass and types of X-ray resources, this review classifies the X-ray binaries and list out their features.

High-Mass X-ray binary: Classification, Formation, and Evolution