High-Mass X-ray binary: Classification, Formation, and Evolution
نویسندگان
چکیده
A high mass X-ray binary is a system consisting of an accreting neutron star or black hole and early-type with more than 10 solar masses. compact produces radiation during the accretion material from stellar wind Roche lobe. High-mass binaries are ideal places to study dense stars, winds, exchange between evolution massive stars. In this review, observational properties, classification, X described. According types resources, review classifies list out their features.
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ژورنال
عنوان ژورنال: Journal of Physics: Conference Series
سال: 2021
ISSN: ['1742-6588', '1742-6596']
DOI: https://doi.org/10.1088/1742-6596/2012/1/012119