Institutional Repository of Radio Astronomy Research Laboratory
| Extended Corbet Diagram of HMXBs, LMXBs and radio pulsar binaries | |
Yan Yan1,3 ; Ali Esamdin1; Yin HongXing2
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| 2010-09-01 | |
| Source Publication | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
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| ISSN | 1674-7348 |
| Volume | 53Issue:9Pages:1726-1731 |
| Contribution Rank | 1 |
| Abstract | The evolutionary scenario of neutron star binaries is still an essential enigma in both stellar astrophysics and high energy astrophysics. In order to explore the scenario, we include the accumulation of data on the orbits and spins of compact binaries in multi-wavelength ranging from radio to X-ray, such as radio pulsar binaries, HMXBs, and LMXBs, filling them into the so called "Corbet Diagram" which initially investigated the period of orbit (P (orb))similar to the period of spin (P (spin)) correlation of HMXBs. We find that the evolutionary scenario comes more clearly and makes strong confirmation of the connection between LMXBs and radio pulsar binaries, predicted by the recycle process. However, the origins of radio pulsar binaries sre still unknown. Accretion Induced Collapse (AIP) process may be a mechanism which can explain the origin of the binary millisecond pulsars with relatively longer orbital periods. A correlation of P (orb) (1/3) similar to P (spin) (-1) of LMXBs and radio pulsar binaries may exist. |
| Keyword | Neutron Star X-ray Binary Pulsar |
| Subtype | Article |
| Subject Area | 致密天体、高能和基础物理 |
| DOI | 10.1007/s11433-010-4064-4 |
| WOS Headings | Science & Technology ; Physical Sciences |
| URL | 查看原文 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | X-RAY BINARIES ; ACCRETION-INDUCED COLLAPSE ; MILLISECOND PULSARS ; LOW-MASS ; GLOBULAR-CLUSTERS ; MAGELLANIC CLOUDS ; ORBITAL PERIOD ; STAR BINARIES ; NEUTRON-STARS ; 4TH EDITION |
| Funding Project | 脉冲星研究团组 |
| WOS Research Area | Physics |
| WOS Subject | Physics, Multidisciplinary |
| WOS ID | WOS:000280810000021 |
| Funding Organization | National Natural Science Foundation of China (Grant Nos. 10573026 and 10773017) ; Program of the Light in China’s Western Region (LCWR) (Grant No. LHXZ200602) ; KnowledgeInnovation Program of the Chinese Academy of Science (Grant No. KJCX2-YW-T09) ; National Basic Research Program of China (Grant No.2009CB824800). |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/76 |
| Collection | 射电天文研究室_脉冲星研究团组 光学天文与技术应用研究室 研究生学位论文 |
| Corresponding Author | Yan Yan |
| Affiliation | 1.Chinese Acad Sci, Urumqi Observ, Natl Astron Observ, Urumqi 830011, Peoples R China 2.Shandong Univ, Sch Space Sci & Phys, Weihai 264209, Peoples R China 3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Yan Yan,Ali Esamdin,Yin HongXing. Extended Corbet Diagram of HMXBs, LMXBs and radio pulsar binaries[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2010,53(9):1726-1731. |
| APA | Yan Yan,Ali Esamdin,&Yin HongXing.(2010).Extended Corbet Diagram of HMXBs, LMXBs and radio pulsar binaries.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,53(9),1726-1731. |
| MLA | Yan Yan,et al."Extended Corbet Diagram of HMXBs, LMXBs and radio pulsar binaries".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 53.9(2010):1726-1731. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Extended Corbet Diag（319KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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