| The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3 | |
Yang, Jun1; García, Federico2; Palacio, Santiago del1; Spencer, Ralph3; Paragi, Zsolt4; Segura, Noel Castro5; Gong, Biping6; Cao, Hongmin7; Chen W(陈文)8,9
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| 发表期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 2023-11 | |
| 卷号 | 526期号:1页码:L1-L7 |
| DOI | 10.1093/mnrasl/slad111 |
| 产权排序 | 第8完成单位 |
| 收录类别 | SCI |
| 关键词 | stars: individual: Cygnus X-3 stars: jets radio continuum: stars X-rays: binaries |
| 摘要 | Cygnus X-3 is a high-mass X-ray binary with a compact object accreting matter from a Wolf-Rayet donor star. Recently, it has been revealed by the Imaging X-ray Polarimetry Explorer (IXPE) as a hidden Galactic ultra-luminous X-ray (ULX) source with a luminosity above the Eddington limit, along the direction of a narrow (opening angle less than or similar to 32 degrees) funnel. In between the IXPE observations, we observed Cyg X-3 with the European very long baseline interferometry (VLBI) Network at 22 GHz and the NICER X-ray instrument. To probe possible relations between the X-ray funnel and the potential radio jet from the ULX, we analysed the simultaneous multiwavelength data. Our high-resolution VLBI image reveals an elongated structure with a position angle of -3.2 +/- 0.4 degrees, accurately perpendicular to the direction of the linear X-ray polarization. Because Cyg X-3 was in the radio quiescent state on 2022 November 10, we identify the mas-scale structure as the innermost radio jet. The finding indicates that the radio jet propagates along and within the funnel. Moreover, the jet is marginally resolved in the transverse direction. This possibly results from the strong stellar winds and the rapid orbital motion of the binary system. |
| 资助项目 | EVN[RSY09]; CONICET[PIP 0113]; CONICET[PIBAA 1275]; National Natural Science Foundation of China (NSFC)[11903079]; Hebei Natural Science Foundation of China[A2022408002]; NSFC[U2031116] |
| 项目资助者 | EVN[RSY09] ; CONICET[PIP 0113, PIBAA 1275] ; National Natural Science Foundation of China (NSFC)[11903079] ; Hebei Natural Science Foundation of China[A2022408002] ; NSFC[U2031116] |
| 语种 | 英语 |
| 学科领域 | 天文学 |
| 文章类型 | Article |
| 出版者 | OXFORD UNIV PRESS |
| 出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
| ISSN | 0035-8711 |
| URL | 查看原文 |
| WOS记录号 | WOS:001152583500001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | CYG X-3 ; VLBI OBSERVATIONS ; MICROQUASAR CYGNUS-X-3 ; RELATIVISTIC JET ; RADIO OUTBURST ; HARD STATE ; EXPANSION ; SCALE ; GHZ ; DISCOVERY |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 版本 | 出版稿 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/26439 |
| 专题 | 射电天文研究组 中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden; 2.Instituto Argentino de Radioastronomía (CCT La Plata, CONICET; CICPBA; UNLP), C.C.5, 3.Villa Elisa, Buenos Aires, Argentina; 4.Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, Oxford Rd., Manchester M13 9PL, UK; 5.Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, the Netherlands; 6.School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK; 7.School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China; 8.School of Electronic and Electrical Engineering, Shangqiu Normal University, 298 Wenhua Road, Shangqiu, Henan 476000, China; 9.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, Yunnan, China; 10.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China |
| 推荐引用方式 GB/T 7714 | Yang, Jun,García, Federico,Palacio, Santiago del,et al. The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,526(1):L1-L7. |
| APA | Yang, Jun.,García, Federico.,Palacio, Santiago del.,Spencer, Ralph.,Paragi, Zsolt.,...&陈文.(2023).The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,526(1),L1-L7. |
| MLA | Yang, Jun,et al."The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 526.1(2023):L1-L7. |
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| The innermost jet in（1450KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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