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| On the Formation of PSR J1640+2224: A Neutron Star Born Massive? | |
Deng, Zhu-Ling1,2,3,4,5 ; Gao, Zhi-Fu1,2,3; Li, Xiang-Dong4,5; Shao, Yong4,5
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| 2020-03-20 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 892Issue:1Pages:4 |
| Contribution Rank | 1 |
| Abstract | PSR J1640+2224 is a binary millisecond pulsar (BMSP) with a white dwarf (WD) companion. Recent observations indicate that the WD is very likely to be a similar to 0.7 M CO WD. Thus, the BMSP should have evolved from an intermediate-mass X-ray binary (IMXB). However, previous investigations on IMXB evolution predict that the orbital periods of the resultant BMSPs are generally < 40 days, in contrast with the 175 day orbital period of PSR J1640+2224. In this paper, we explore the influence of the mass of the neutron star (NS) and the chemical compositions of the companion star on the formation of BMSPs. Our results show that the final orbital period becomes longer with increasing NS mass, and the WD mass becomes larger with decreasing metallicity. In particular, to reproduce the properties of PSR J1640+2224, the NS was likely born massive (>2.0 M). |
| Keyword | Neutron stars Compact binary stars Binary pulsars |
| DOI | 10.3847/1538-4357/ab76c4 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | WHITE-DWARF COMPANIONS ; CLOSE BINARY-SYSTEMS ; MILLISECOND PULSARS ; EVOLUTION ; PERIOD ; ROTATION |
| Funding Project | National Key Research and Development Program of China[2016YFA0400803] ; Natural Science Foundation of China[11773015] ; Natural Science Foundation of China[U1838201] ; Natural Science Foundation of China - CAS[11773015] ; Natural Science Foundation of China - CAS[U1838201] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000521418000001 |
| Publisher | IOP PUBLISHING LTD |
| Funding Organization | National Key Research and Development Program of China ; Natural Science Foundation of China ; Natural Science Foundation of China - CAS |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/3447 |
| Collection | 射电天文研究室_脉冲星研究团组 |
| Corresponding Author | Gao, Zhi-Fu |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 3.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China 4.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China 5.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, 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 | Deng, Zhu-Ling,Gao, Zhi-Fu,Li, Xiang-Dong,et al. On the Formation of PSR J1640+2224: A Neutron Star Born Massive?[J]. ASTROPHYSICAL JOURNAL,2020,892(1):4. |
| APA | Deng, Zhu-Ling,Gao, Zhi-Fu,Li, Xiang-Dong,&Shao, Yong.(2020).On the Formation of PSR J1640+2224: A Neutron Star Born Massive?.ASTROPHYSICAL JOURNAL,892(1),4. |
| MLA | Deng, Zhu-Ling,et al."On the Formation of PSR J1640+2224: A Neutron Star Born Massive?".ASTROPHYSICAL JOURNAL 892.1(2020):4. |
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| Deng-2020-On the For（663KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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