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Population synthesis of high mass X-ray binaries
Lue, Guo-Liang1,2; Zhu, Chun-Hua1,2,3; Wang, Zhao-Jun1,2
2011-03-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume11Issue:3Pages:327-334
AbstractBy simulating the evolution of spin periods of magnetized neutron stars which interact with their environment in binary systems, we investigate the Galactic population of high mass X-ray binaries (HMXBs). The number of HMXBs in the Galaxy is between 190 and 240, and their birthrate is from 5.9 x 10(-5) yr(-1) to 6.3 x 10(-5) yr(-1). Comparing the Corbet diagram (the positions of the spin periods vs. the orbital periods of HMXBs) in our model with the associated observations, we find that the stellar wind structure and the process of matter transfer are very important for understanding HMXBs.
KeywordStars: Evolution X-rays: Binaries Galaxy: Stellar Content
SubtypeArticle
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordNEUTRON-STAR ; SYMBIOTIC STARS ; RADIO PULSARS ; EVOLUTION ; COLLAPSE ; GALAXY
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000289448700006
Citation statistics
Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/846
Collection射电天文研究室_脉冲星研究团组
射电天文研究室
其它
Affiliation1.Xinjiang Univ, Sch Phys, Urumqi 830046, Peoples R China
2.Xinjiang Univ Natl Astron Observ Joint Ctr Astrop, Urumqi 830046, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Urumqi Observ, Urumqi 830011, Peoples R China
Recommended Citation
GB/T 7714
Lue, Guo-Liang,Zhu, Chun-Hua,Wang, Zhao-Jun. Population synthesis of high mass X-ray binaries[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2011,11(3):327-334.
APA Lue, Guo-Liang,Zhu, Chun-Hua,&Wang, Zhao-Jun.(2011).Population synthesis of high mass X-ray binaries.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,11(3),327-334.
MLA Lue, Guo-Liang,et al."Population synthesis of high mass X-ray binaries".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 11.3(2011):327-334.
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