Polarization of RRAT J2325-0530 with FAST
文献类型:期刊论文
| 作者 | Yang, Le1,2; Gao, Zhi-Fu1; Wen, Zhi-Gang1; Zhang, Li-Yun2,3; Li, Baoda2; Shan, Hao1 |
| 刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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| 出版日期 | 2025-12-01 |
| 卷号 | 25期号:12页码:17 |
| 关键词 | polarization radiation mechanisms: general (stars:)pulsars: individual(J2325-0530) |
| ISSN号 | 1674-4527 |
| DOI | 10.1088/1674-4527/ae007a |
| 通讯作者 | Gao, Zhi-Fu(zhifugao@xao.ac.cn) ; Wen, Zhi-Gang(wenzhigang@xao.ac.cn) ; Zhang, Li-Yun(liy_zhang@hotmail.com) |
| 英文摘要 | We report on high-sensitivity polarization measurements of the rotating radio transient (RRAT) J2325-0530 conducted with the Five-hundred-meter Aperture Spherical radio Telescope. Using single-pulse search techniques and full-Stokes parameter analysis, we comprehensively explore the source's emission characteristics. The observations reveal three distinct pulse profile types-single-peaked, double-peaked, and multi-peaked-with the multi-peaked category displaying prominent polarization reversals (mean linear polarization fraction of 27.5% +/- 0.3%) and broader pulse widths ( 7.degrees 50 +/- 0.degrees 82 ). The relative pulse energy distribution follows a power-law trend and exhibits a strong positive correlation with pulse width (r = 0.80). Through analysis of orthogonal polarization mode transitions, we suggest that the emission likely results from the interplay of multi-scale magnetospheric processes in the polar cap region. Future multi-wavelength campaigns could further test the distinctiveness of this source's emission mechanism. Overall, our findings enhance the current understanding of RRATs' complex emission behavior and inform the broader study of pulsar magnetospheric dynamics. |
| WOS关键词 | ROTATING RADIO TRANSIENTS ; PULSAR MAGNETOSPHERES ; CURVATURE RADIATION ; GREEN BANK ; EMISSION ; PROPAGATION ; STATISTICS ; DISCOVERY ; TIME |
| 资助项目 | Chinese Academy of Sciences (CAS)[PT2021_0117] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001600387100001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | Chinese Academy of Sciences (CAS) |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/8277] ![]() |
| 专题 | 脉冲星研究团组 |
| 通讯作者 | Gao, Zhi-Fu; Wen, Zhi-Gang; Zhang, Li-Yun |
| 作者单位 | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Guizhou Univ, Coll Phys, Guiyang 550025, Peoples R China 3.Int Ctr Supernovae, Yunnan Key Lab, Kunming 650216, Peoples R China |
| 推荐引用方式 GB/T 7714 | Yang, Le,Gao, Zhi-Fu,Wen, Zhi-Gang,et al. Polarization of RRAT J2325-0530 with FAST[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2025,25(12):17. |
| APA | Yang, Le,Gao, Zhi-Fu,Wen, Zhi-Gang,Zhang, Li-Yun,Li, Baoda,&Shan, Hao.(2025).Polarization of RRAT J2325-0530 with FAST.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,25(12),17. |
| MLA | Yang, Le,et al."Polarization of RRAT J2325-0530 with FAST".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 25.12(2025):17. |
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来源:新疆天文台
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