Institutional Repository of Radio Astronomy Research Laboratory
| Studying the Radio Eclipse of Spider Pulsar J1816+4510 with the FAST | |
Shang, Lunhua1,2,3; Yu, Yan1,2; Dang, Shijun1,2 ; Bai, Juntao4,5; Xu, Xin1,2; Wang, Shuangqiang4; Zhi, Qijun1,2; Dong, Aijun1,2; Pang, Lijun1; Li, Qingying1,2; Qiao, Guojun6
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| 2024-07-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 969Issue:1Pages:62 |
| Contribution Rank | 4 |
| Abstract | We report on the radio eclipse properties of spider pulsar J1816+4510 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The high-sensitivity FAST observations will allow us to probe much deeper into the eclipse region of this pulsar at higher frequencies >1 GHz. The duration of the full eclipse, eclipse ingress, and egress at 1100, 1200, 1300, and 1400 MHz are measured, respectively. The variation of eclipse duration with frequency is studied by splitting the FAST observations into four subbands. It is found that the eclipse egress of PSR J1816+4510 takes longer than the ingress and becomes more symmetrical with increasing frequency. The variations of the durations with the frequency for the full eclipse, eclipse ingress, and egress follow a power-law decay pattern with different indices. The pulse profile variations near the eclipse are studied. It is found that the broadening of pulse profiles becomes more prominent with deepening into the eclipse region due to the scattering from the companion star. Moreover, the pulse smearing induced by the scattering and the rapid dispersion measure (DM) fluctuations within a subintegration during the eclipse egress at different frequencies and orbital phases is comparatively studied. It is found that the scattering plays a more important role than the DM fluctuations for the pulse smearing of the eclipse. The observations of this paper will provide important clues for the theoretical studies of the radio eclipse mechanism of the spider pulsar systems. |
| DOI | 10.3847/1538-4357/ad4961 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | MILLISECOND PULSAR ; BINARY ; EVOLUTION ; DISCOVERY ; FREQUENCY ; PSRCHIVE ; PSRFITS ; DECADE ; MODEL |
| Funding Project | Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-3] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[2022A03013-4] ; Academic New Seedling Fund Project of Guizhou Normal University[[2022]B18] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]137] ; Scientific Research Project of the Guizhou Provincial Education[KY[2022]132] ; Guizhou Provincial Science and Technology Foundation[ZK[2022]304] ; National Natural Science Foundation of China (NSFC) project[12203092] ; National Natural Science Foundation of China (NSFC) project[12273008] ; National Natural Science Foundation of China (NSFC) project[12363005] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[2022D01B71] ; National SKA Program of China[2020SKA0120100] ; National SKA Program of China[2022SKA0130100] ; National SKA Program of China[2022SKA0130104] ; Natural Science and Technology Foundation of Guizhou Province[[2023]024] ; Foundation of Guizhou Provincial Education Department[KY(2020)003] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001260176600001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Academic New Seedling Fund Project of Guizhou Normal University ; Scientific Research Project of the Guizhou Provincial Education ; Guizhou Provincial Science and Technology Foundation ; National Natural Science Foundation of China (NSFC) project ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; National SKA Program of China ; Natural Science and Technology Foundation of Guizhou Province ; Foundation of Guizhou Provincial Education Department |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6814 |
| Collection | 射电天文研究室_脉冲星研究团组 科研仪器设备产出_我台利用FAST观测数据文章 |
| Corresponding Author | Shang, Lunhua; Dang, Shijun; Bai, Juntao |
| Affiliation | 1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China 2.Guizhou Normal Univ, Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 5.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 6.Peking Univ, Sch Phys, 5 Yihe yuan Rd, Beijing 100871, Peoples R China |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Shang, Lunhua,Yu, Yan,Dang, Shijun,et al. Studying the Radio Eclipse of Spider Pulsar J1816+4510 with the FAST[J]. ASTROPHYSICAL JOURNAL,2024,969(1):62. |
| APA | Shang, Lunhua.,Yu, Yan.,Dang, Shijun.,Bai, Juntao.,Xu, Xin.,...&Qiao, Guojun.(2024).Studying the Radio Eclipse of Spider Pulsar J1816+4510 with the FAST.ASTROPHYSICAL JOURNAL,969(1),62. |
| MLA | Shang, Lunhua,et al."Studying the Radio Eclipse of Spider Pulsar J1816+4510 with the FAST".ASTROPHYSICAL JOURNAL 969.1(2024):62. |
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| Shang-2024-Studying （1648KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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