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Constraints from luminosity-displacement correlation of high-mass X-ray binaries

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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We have modeled the luminosity-displacement correlation of high-mass X-ray binaries (HMXBs) with an evolutionary population synthesis (EPS) code. Detailed properties including offsets of simulated HMXBs are presented under both common envelope prescriptions usually adopted (i.e., the αCE formalism and the γ algorithm), and several theoretical models describing the natal kicks. We suggest that the distinct observational properties may be used as potential evidence to discriminate between models.

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. 337 - 341
Copyright
© International Astronomical Union 2019 

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