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High-mass X-ray binaries: Evolutionary population synthesis modeling
| Content Provider | Scilit |
|---|---|
| Author | Zuo, Zhao-Yu |
| Copyright Year | 2018 |
| Description | 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 $α_{CE}$ 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. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/3D1EEFBE51E042A1C480C80FEA91750E/S1743921318007457a.pdf/div-class-title-high-mass-x-ray-binaries-evolutionary-population-synthesis-modeling-div.pdf |
| Ending Page | 458 |
| Page Count | 4 |
| Starting Page | 455 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921318007457 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S346 |
| Volume Number | 14 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2018-08-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics Stellar Evolution Compact Stars ray Binaries |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
