Precision Determination of Scintillation Screen Parameters from Annual Modulation Measurement of Pulsar Scintillation Arc Curvature with the FAST Telescope
文献类型:期刊论文
| 作者 | Huang, Yuanshang2; Shi, Xun2; Yao, Jumei1,7,8; Zhu, Weiwei5,6; Xu, Yonghua3,4 |
| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2026-01-20 |
| 卷号 | 997期号:1页码:131 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/ae25e4 |
| 产权排序 | 2 |
| 英文摘要 | Pulsar scintillation observations have revealed ubiquitous discrete scintillation screens in the interstellar medium. A major obstacle in identifying the nature of these screens is the uncertainty in their distances, which prevents precise correlation with known structures in the Milky Way. We used the Five-hundred-meter Aperture Spherical radio Telescope to observe PSR B1237+25, PSR 1842+14, and PSR 2021+51. We detected 10 scintillation arcs in PSR B1237+25, 1 in PSR 1842+14, and at least 6 in PSR 2021+51. By modeling the annual modulation of these scintillation arcs, we constrained the distances of the scintillation screens, as well as the anisotropic scattering directions and the projected velocities in those directions. The scintillation screens are distributed throughout the entire paths between Earth and the pulsars. Among these, the distance to the main scintillation screen toward PSR B1237+25 is 267-28+32 pc, the scintillation screen toward PSR B1842+14 is at a distance of 240-120+210 pc, and the main scintillation screen toward PSR B2021+51 is located at 887-132+167 pc. Several screens in our sample appear at distances coinciding with the Local Bubble boundary, particularly the brightest scintillation arc toward PSR B1237+25. We provide a substantial sample of scintillation screen measurements, revealing the rich plasma density fluctuation structures present in the Milky Way. |
| WOS关键词 | INTERSTELLAR-MEDIUM ; EMISSION REGIONS ; PARABOLIC ARCS ; PLASMA LENSES ; NEUTRON-STARS ; BOW SHOCKS ; SCATTERING ; ASTROPY ; SCINTILLOMETRY ; PACKAGE |
| 资助项目 | MOST divided by National Natural Science Foundation of China (NSFC)[12373025] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001664601400001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | MOST divided by National Natural Science Foundation of China (NSFC) |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/8499] ![]() |
| 专题 | 脉冲星研究团组 |
| 通讯作者 | Huang, Yuanshang; Shi, Xun |
| 作者单位 | 1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1-St, Urumqi 830011, Xinjiang, Peoples R China 2.Yunnan Univ, South Western Inst Astron Res SWIFAR, Kunming 650500, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron & Technol, Beijing 100101, Peoples R China 4.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China 5.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China 6.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 7.Xinjiang Key Lab Radio Astrophys, 150 Sci 1-St, Urumqi 830011, Xinjiang, Peoples R China 8.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China |
| 推荐引用方式 GB/T 7714 | Huang, Yuanshang,Shi, Xun,Yao, Jumei,et al. Precision Determination of Scintillation Screen Parameters from Annual Modulation Measurement of Pulsar Scintillation Arc Curvature with the FAST Telescope[J]. ASTROPHYSICAL JOURNAL,2026,997(1):131. |
| APA | Huang, Yuanshang,Shi, Xun,Yao, Jumei,Zhu, Weiwei,&Xu, Yonghua.(2026).Precision Determination of Scintillation Screen Parameters from Annual Modulation Measurement of Pulsar Scintillation Arc Curvature with the FAST Telescope.ASTROPHYSICAL JOURNAL,997(1),131. |
| MLA | Huang, Yuanshang,et al."Precision Determination of Scintillation Screen Parameters from Annual Modulation Measurement of Pulsar Scintillation Arc Curvature with the FAST Telescope".ASTROPHYSICAL JOURNAL 997.1(2026):131. |
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来源:新疆天文台
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