Investigation of some physical properties of accretion induced collapse in producing millisecond pulsars
文献类型:期刊论文
作者 | Taani, Ali2; Zhang, Chengmin2![]() ![]() |
刊名 | ASTROPHYSICS AND SPACE SCIENCE
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出版日期 | 2012-07-01 |
卷号 | 340期号:1页码:147-153 |
关键词 | Stars: neutron stars White dwarfs Cataclysmic variables X-ray binaries Fundamental parameters |
英文摘要 | We investigate some physical characteristics of Millisecond Pulsars (MSPs) such as magnetic fields, spin periods and masses, that are produced by Accretion Induced Collapse (AIC) of an accreting white dwarf (WD) in stellar binary systems. We also investigate the changes of these characteristics during the mass-transfer phase of the system in its way to become a MSP. Our approach allows us to follow the changes in magnetic fields and spin periods during the conversion of WDs to MSPs via AIC process. We focus our attention mainly on the massive binary WDs (Ma parts per thousand(3)1.0M (aS (TM))) forming cataclysmic variables, that could potentially evolve to reach Chandrasekhar limit, thereafter they collapse and become MSPs. Knowledge about these parameters might be useful for further modeling of the observed features of AIC. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000304609800017 |
源URL | [http://ir.bao.ac.cn/handle/114a11/6290] ![]() |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Al Hussein Bin Talal Univ, Dept Phys, Maan 71111, Jordan 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 3.Yarmouk Univ, Dept Phys, Irbid 21163, Jordan |
推荐引用方式 GB/T 7714 | Taani, Ali,Zhang, Chengmin,Al-Wardat, Mashhoor,et al. Investigation of some physical properties of accretion induced collapse in producing millisecond pulsars[J]. ASTROPHYSICS AND SPACE SCIENCE,2012,340(1):147-153. |
APA | Taani, Ali,Zhang, Chengmin,Al-Wardat, Mashhoor,&Zhao, Yongheng.(2012).Investigation of some physical properties of accretion induced collapse in producing millisecond pulsars.ASTROPHYSICS AND SPACE SCIENCE,340(1),147-153. |
MLA | Taani, Ali,et al."Investigation of some physical properties of accretion induced collapse in producing millisecond pulsars".ASTROPHYSICS AND SPACE SCIENCE 340.1(2012):147-153. |
入库方式: OAI收割
来源:国家天文台
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