| NICER, NuSTAR, and Insight-HXMT Views to the Newly Discovered Black Hole X-Ray Binary Swift J1727.8-1613 | |
Peng, Jing-Qiang1,2; Zhang, Shu1; Shui, Qing-Cang1,2; Zhang, Shuang-Nan1,2; Kong, Ling-Da3; Chen, Yu-Peng1; Wang, Peng-Ju3; Ji, Long4; Qu, Jin-Lu1; Tao, Lian1; Ge, Ming-Yu1; Chang, Zhi1; Li, Jian5,6; Li, Zhao-sheng7; Yu, Zhuo-Li1; Yan Z(颜哲)2,8,9,10
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| 发表期刊 | ASTROPHYSICAL JOURNAL LETTERS
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| 2024 | |
| 卷号 | 960期号:2 |
| DOI | 10.3847/2041-8213/ad17ca |
| 产权排序 | 第8完成单位 |
| 收录类别 | SCI |
| 摘要 | Swift J1727.8-1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR observations when the source was approaching the hard intermediate state. Such a joint view reveals an additional hard component apart from the normally observed hard component with reflection in the spectrum, to be distinguished from the usual black hole X-ray binary systems. By including this extra component in the spectrum, we have measured a high spin of 0.98-0.07+0.02 and an inclination of around 40-0.8+1.2 degrees, which is consistent with NICER results reported before. However, we find that the additional spectral component cannot be exclusively determined due to the model degeneracy. Accordingly, a possible jet/corona configuration is adjusted to account for the spectral fitting with different model trials. The extra component may originate either from a relativistic jet or a jet base/corona underneath a slow jet. |
| 资助项目 | National Key R&D Program of China[2021YFA0718500] ; National Natural Science Foundation of China[U1838201] ; National Natural Science Foundation of China[U1838202] ; National Natural Science Foundation of China[U2038101] ; National Natural Science Foundation of China[U1938103] ; National Natural Science Foundation of China[12273030] ; National Natural Science Foundation of China[U1938107] ; China National Space Administration (CNSA) ; Chinese Academy of Sciences(CAS) ; International Partnership Program of the Chinese Academy of Sciences[113111KYSB20190020] ; NASAs Goddard Space Flight Center ; Sino-German (CSC-DAAD) Postdoc Scholarship Program[57251553] |
| 项目资助者 | National Key R&D Program of China[2021YFA0718500] ; National Natural Science Foundation of China[U1838201, U1838202, U2038101, U1938103, 12273030, U1938107] ; China National Space Administration (CNSA) ; Chinese Academy of Sciences(CAS) ; International Partnership Program of the Chinese Academy of Sciences[113111KYSB20190020] ; NASAs Goddard Space Flight Center ; Sino-German (CSC-DAAD) Postdoc Scholarship Program[57251553] |
| 语种 | 英语 |
| 学科领域 | 天文学 |
| 文章类型 | Article |
| 出版者 | IOP Publishing Ltd |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 2041-8205 |
| URL | 查看原文 |
| WOS记录号 | WOS:001139762500001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | ACCRETION DISK ; ENERGY ; EVOLUTION ; REFLECTION ; SPECTRUM ; SPIN ; INSTABILITY ; MODEL ; STATE |
| 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/114a53/26489 |
| 专题 | 高能天体物理研究组 中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 100049, Beijing, People's Republic of China [email protected], [email protected], [email protected]; 2.University of Chinese Academy of Sciences, Chinese Academy of Sciences, 100049, Beijing, People's Republic of China; 3.Institute für Astronomie und Astrophysik, Kepler Center for Astro and Particle Physics, Eberhard Karls, Universität, Sand 1, D-72076 Tübingen, Germany; 4.School of Physics and Astronomy, Sun Yat-Sen University, Zhuhai, 519082, People's Republic of China; 5.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, People's Republic of China; 6.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People's Republic of China; 7.Key Laboratory of Stars and Interstellar Medium, Xiangtan University, Xiangtan 411105, Hunan, People's Republic of China; 8.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 9.Key Laboratory for the Structure and Evolution Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 10.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Peng, Jing-Qiang,Zhang, Shu,Shui, Qing-Cang,et al. NICER, NuSTAR, and Insight-HXMT Views to the Newly Discovered Black Hole X-Ray Binary Swift J1727.8-1613[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,960(2). |
| APA | Peng, Jing-Qiang.,Zhang, Shu.,Shui, Qing-Cang.,Zhang, Shuang-Nan.,Kong, Ling-Da.,...&Yan Z.(2024).NICER, NuSTAR, and Insight-HXMT Views to the Newly Discovered Black Hole X-Ray Binary Swift J1727.8-1613.ASTROPHYSICAL JOURNAL LETTERS,960(2). |
| MLA | Peng, Jing-Qiang,et al."NICER, NuSTAR, and Insight-HXMT Views to the Newly Discovered Black Hole X-Ray Binary Swift J1727.8-1613".ASTROPHYSICAL JOURNAL LETTERS 960.2(2024). |
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| NICER, NuSTAR, and I（2460KB） | 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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