Comparing the Observational Properties of Rotation-Powered Binary Millisecond Pulsars with Various Companion Types
文献类型：期刊论文
| 作者 | Wang, De-Hua1; Zhang, Cheng-Min3,4,5; Wang, Shuang-Qiang2 |
| 刊名 | UNIVERSE
 |
| 出版日期 | 2025-09-19 |
| 卷号 | 11期号:9页码:321 |
| 关键词 | (stars:) pulsars: general stars: neutron (stars:) binaries: general gamma rays: stars |
| DOI | 10.3390/universe11090321 |
| 产权排序 | 5 |
| 英文摘要 | We compare the observational properties of rotation-powered binary millisecond pulsars (BMSPs) in the Galactic Field with various companion types. First, BMSPs with diverse companion types exhibit different properties in the relation of binary orbital period versus companion mass, and in the spin period distribution of neutron stars (NSs), etc., implying multiple origins of BMSPs. Second, BMSPs with companions of CO/ONeMg white dwarfs (CO-BMSPs) show fewer sources than those with companions of Helium white dwarfs (He-BMSPs), which may result from the different evolutionary histories or accretion efficiencies in their progenitors. Third, BMSPs with main-sequence companions (MS-BMSPs) and ultra-light companions or planets (UL-BMSPs) are mostly eclipsing sources that are detected in both radio and gamma-ray bands (i.e., radio+gamma sources), implying that they may be younger systems and share a faster average spin period and higher average accretion rate than CO-BMSPs/He-BMSPs. We propose that the predecessors of MS-BMSPs may share a short binary orbital distance with low-mass companion stars of M-c similar to 0.5-0.8M(circle dot), which induces an efficient binary accretion process, and ultimately leaves a BMSP with a main-sequence companion due to the low efficiency of its hydrogen burning. Lastly, radio+gamma He-BMSPs share a faster average spin period of NSs than radio-only He-BMSPs. Meanwhile, these two groups of sources share similar companion mass distributions, implying the gamma-ray evaporation effect may not obviously strip the companion mass of He-BMSPs during similar to 0.3 Gyr, which may be due to the strong gravitational potential energy of the white dwarf companions. |
| WOS关键词 | WHITE-DWARF COMPANIONS ; LOW-MASS STARS ; X-RAY ; EVOLUTION ; RADIO ; ACCRETION ; IRRADIATION ; EMISSION ; FIELD ; AGES |
| 资助项目 | National Natural Science Foundation of China ; [12163001] ; [12463007] |
| WOS研究方向 | Astronomy & Astrophysics ; Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:001582250900001 |
| 出版者 | MDPI |
| 资助机构 | National Natural Science Foundation of China |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/8190]  |
| 专题 | 脉冲星研究团组 |
| 通讯作者 | Wang, De-Hua; Zhang, Cheng-Min |
| 作者单位 | 1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550025, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron, Beijing 100101, Peoples R China 4.Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China 5.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing 100101, Peoples R China |
| 推荐引用方式 GB/T 7714 | Wang, De-Hua,Zhang, Cheng-Min,Wang, Shuang-Qiang. Comparing the Observational Properties of Rotation-Powered Binary Millisecond Pulsars with Various Companion Types[J]. UNIVERSE,2025,11(9):321. |
| APA | Wang, De-Hua,Zhang, Cheng-Min,&Wang, Shuang-Qiang.(2025).Comparing the Observational Properties of Rotation-Powered Binary Millisecond Pulsars with Various Companion Types.UNIVERSE,11(9),321. |
| MLA | Wang, De-Hua,et al."Comparing the Observational Properties of Rotation-Powered Binary Millisecond Pulsars with Various Companion Types".UNIVERSE 11.9(2025):321. |
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