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High-mass X-ray binaries: Evolutionary population synthesis modeling

Published online by Cambridge University Press:  30 December 2019

Zhao-yu Zuo
Zhao-yu Zuo*
Affiliation:
School of Science, Xi’an Jiaotong University, Xi’an 710049, China email: zuozyu@xjtu.edu.cn
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Abstract

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Using an evolutionary population synthesis code, we modeled the universal, featureless X-ray luminosity function of high-mass X-ray binaries (HMXBs) in star-forming galaxies. We put constraints on the natal kicks, super-Eddington accretion factor, as well as common envelope prescriptions usually adopted (i.e., the αCE formalism and the γ algorithm), and presented the detailed properties of HMXBs under different models, which may be investigated further by future high-resolution X-ray and optical observations.

Keywords

stellar evolutioncompact starsX-ray binaries
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 455 - 458
Copyright
© International Astronomical Union 2019 

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