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Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070
A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each other. However, such an evolution is still unclear in both its geometry and dynamics. Here we report the unusual decrease...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2021
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7884741/ https://www.ncbi.nlm.nih.gov/pubmed/33589623 http://dx.doi.org/10.1038/s41467-021-21169-5 |
| _version_ | 1783651475059113984 |
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| author | You, Bei Tuo, Yuoli Li, Chengzhe Wang, Wei Zhang, Shuang-Nan Zhang, Shu Ge, Mingyu Luo, Chong Liu, Bifang Yuan, Weimin Dai, Zigao Liu, Jifeng Qiao, Erlin Jin, Chichuan Liu, Zhu Czerny, Bozena Wu, Qingwen Bu, Qingcui Cai, Ce Cao, Xuelei Chang, Zhi Chen, Gang Chen, Li Chen, Tianxiang Chen, Yibao Chen, Yong Chen, Yupeng Cui, Wei Cui, Weiwei Deng, Jingkang Dong, Yongwei Du, Yuanyuan Fu, Minxue Gao, Guanhua Gao, He Gao, Min Gu, Yudong Guan, Ju Guo, Chengcheng Han, Dawei Huang, Yue Huo, Jia Jia, Shumei Jiang, Luhua Jiang, Weichun Jin, Jing Jin, Yongjie Kong, Lingda Li, Bing Li, Chengkui Li, Gang Li, Maoshun Li, Tipei Li, Wei Li, Xian Li, Xiaobo Li, Xufang Li, Yanguo Li, Zhengwei Liang, Xiaohua Liao, Jinyuan Liu, Congzhan Liu, Guoqing Liu, Hongwei Liu, Xiaojing Liu, Yinong Lu, Bo Lu, Fangjun Lu, Xuefeng Luo, Qi Luo, Tao Ma, Xiang Meng, Bin Nang, Yi Nie, Jianyin Ou, Ge Qu, Jinlu Sai, Na Shang, Rencheng Song, Liming Song, Xinying Sun, Liang Tan, Ying Tao, Lian Wang, Chen Wang, Guofeng Wang, Juan Wang, Lingjun Wang, Wenshuai Wang, Yusa Wen, Xiangyang Wu, Baiyang Wu, Bobing Wu, Mei Xiao, Guangcheng Xiao, Shuo Xiong, Shaolin Xu, Yupeng Yang, Jiawei Yang, Sheng Yang, Yanji Yi, Qibin Yin, Qianqing You, Yuan Zhang, Aimei Zhang, Chengmo Zhang, Fan Zhang, Hongmei Zhang, Juan Zhang, Tong Zhang, Wanchang Zhang, Wei Zhang, Wenzhao Zhang, Yi Zhang, Yifei Zhang, Yongjie Zhang, Yue Zhang, Zhao Zhang, Ziliang Zhao, Haisheng Zhao, Xiaofan Zheng, Shijie Zhou, Dengke Zhou, Jianfeng Zhu, Yuxuan Zhu, Yue |
| author_facet | You, Bei Tuo, Yuoli Li, Chengzhe Wang, Wei Zhang, Shuang-Nan Zhang, Shu Ge, Mingyu Luo, Chong Liu, Bifang Yuan, Weimin Dai, Zigao Liu, Jifeng Qiao, Erlin Jin, Chichuan Liu, Zhu Czerny, Bozena Wu, Qingwen Bu, Qingcui Cai, Ce Cao, Xuelei Chang, Zhi Chen, Gang Chen, Li Chen, Tianxiang Chen, Yibao Chen, Yong Chen, Yupeng Cui, Wei Cui, Weiwei Deng, Jingkang Dong, Yongwei Du, Yuanyuan Fu, Minxue Gao, Guanhua Gao, He Gao, Min Gu, Yudong Guan, Ju Guo, Chengcheng Han, Dawei Huang, Yue Huo, Jia Jia, Shumei Jiang, Luhua Jiang, Weichun Jin, Jing Jin, Yongjie Kong, Lingda Li, Bing Li, Chengkui Li, Gang Li, Maoshun Li, Tipei Li, Wei Li, Xian Li, Xiaobo Li, Xufang Li, Yanguo Li, Zhengwei Liang, Xiaohua Liao, Jinyuan Liu, Congzhan Liu, Guoqing Liu, Hongwei Liu, Xiaojing Liu, Yinong Lu, Bo Lu, Fangjun Lu, Xuefeng Luo, Qi Luo, Tao Ma, Xiang Meng, Bin Nang, Yi Nie, Jianyin Ou, Ge Qu, Jinlu Sai, Na Shang, Rencheng Song, Liming Song, Xinying Sun, Liang Tan, Ying Tao, Lian Wang, Chen Wang, Guofeng Wang, Juan Wang, Lingjun Wang, Wenshuai Wang, Yusa Wen, Xiangyang Wu, Baiyang Wu, Bobing Wu, Mei Xiao, Guangcheng Xiao, Shuo Xiong, Shaolin Xu, Yupeng Yang, Jiawei Yang, Sheng Yang, Yanji Yi, Qibin Yin, Qianqing You, Yuan Zhang, Aimei Zhang, Chengmo Zhang, Fan Zhang, Hongmei Zhang, Juan Zhang, Tong Zhang, Wanchang Zhang, Wei Zhang, Wenzhao Zhang, Yi Zhang, Yifei Zhang, Yongjie Zhang, Yue Zhang, Zhao Zhang, Ziliang Zhao, Haisheng Zhao, Xiaofan Zheng, Shijie Zhou, Dengke Zhou, Jianfeng Zhu, Yuxuan Zhu, Yue |
| author_sort | You, Bei |
| collection | PubMed |
| description | A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each other. However, such an evolution is still unclear in both its geometry and dynamics. Here we report the unusual decrease of the reflection fraction in MAXI J1820+070, which is the ratio of the coronal intensity illuminating the disk to the coronal intensity reaching the observer, as the corona is observed to contrast during the decay phase. We postulate a jet-like corona model, in which the corona can be understood as a standing shock where the material flowing through. In this dynamical scenario, the decrease of the reflection fraction is a signature of the corona’s bulk velocity. Our findings suggest that as the corona is observed to get closer to the black hole, the coronal material might be outflowing faster. |
| format | Online Article Text |
| id | pubmed-7884741 |
| institution | National Center for Biotechnology Information |
| language | English |
| publishDate | 2021 |
| publisher | Nature Publishing Group UK |
| record_format | MEDLINE/PubMed |
| spelling | pubmed-78847412021-02-25 Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 You, Bei Tuo, Yuoli Li, Chengzhe Wang, Wei Zhang, Shuang-Nan Zhang, Shu Ge, Mingyu Luo, Chong Liu, Bifang Yuan, Weimin Dai, Zigao Liu, Jifeng Qiao, Erlin Jin, Chichuan Liu, Zhu Czerny, Bozena Wu, Qingwen Bu, Qingcui Cai, Ce Cao, Xuelei Chang, Zhi Chen, Gang Chen, Li Chen, Tianxiang Chen, Yibao Chen, Yong Chen, Yupeng Cui, Wei Cui, Weiwei Deng, Jingkang Dong, Yongwei Du, Yuanyuan Fu, Minxue Gao, Guanhua Gao, He Gao, Min Gu, Yudong Guan, Ju Guo, Chengcheng Han, Dawei Huang, Yue Huo, Jia Jia, Shumei Jiang, Luhua Jiang, Weichun Jin, Jing Jin, Yongjie Kong, Lingda Li, Bing Li, Chengkui Li, Gang Li, Maoshun Li, Tipei Li, Wei Li, Xian Li, Xiaobo Li, Xufang Li, Yanguo Li, Zhengwei Liang, Xiaohua Liao, Jinyuan Liu, Congzhan Liu, Guoqing Liu, Hongwei Liu, Xiaojing Liu, Yinong Lu, Bo Lu, Fangjun Lu, Xuefeng Luo, Qi Luo, Tao Ma, Xiang Meng, Bin Nang, Yi Nie, Jianyin Ou, Ge Qu, Jinlu Sai, Na Shang, Rencheng Song, Liming Song, Xinying Sun, Liang Tan, Ying Tao, Lian Wang, Chen Wang, Guofeng Wang, Juan Wang, Lingjun Wang, Wenshuai Wang, Yusa Wen, Xiangyang Wu, Baiyang Wu, Bobing Wu, Mei Xiao, Guangcheng Xiao, Shuo Xiong, Shaolin Xu, Yupeng Yang, Jiawei Yang, Sheng Yang, Yanji Yi, Qibin Yin, Qianqing You, Yuan Zhang, Aimei Zhang, Chengmo Zhang, Fan Zhang, Hongmei Zhang, Juan Zhang, Tong Zhang, Wanchang Zhang, Wei Zhang, Wenzhao Zhang, Yi Zhang, Yifei Zhang, Yongjie Zhang, Yue Zhang, Zhao Zhang, Ziliang Zhao, Haisheng Zhao, Xiaofan Zheng, Shijie Zhou, Dengke Zhou, Jianfeng Zhu, Yuxuan Zhu, Yue Nat Commun Article A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each other. However, such an evolution is still unclear in both its geometry and dynamics. Here we report the unusual decrease of the reflection fraction in MAXI J1820+070, which is the ratio of the coronal intensity illuminating the disk to the coronal intensity reaching the observer, as the corona is observed to contrast during the decay phase. We postulate a jet-like corona model, in which the corona can be understood as a standing shock where the material flowing through. In this dynamical scenario, the decrease of the reflection fraction is a signature of the corona’s bulk velocity. Our findings suggest that as the corona is observed to get closer to the black hole, the coronal material might be outflowing faster. Nature Publishing Group UK 2021-02-15 /pmc/articles/PMC7884741/ /pubmed/33589623 http://dx.doi.org/10.1038/s41467-021-21169-5 Text en © The Author(s) 2021 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/. |
| spellingShingle | Article You, Bei Tuo, Yuoli Li, Chengzhe Wang, Wei Zhang, Shuang-Nan Zhang, Shu Ge, Mingyu Luo, Chong Liu, Bifang Yuan, Weimin Dai, Zigao Liu, Jifeng Qiao, Erlin Jin, Chichuan Liu, Zhu Czerny, Bozena Wu, Qingwen Bu, Qingcui Cai, Ce Cao, Xuelei Chang, Zhi Chen, Gang Chen, Li Chen, Tianxiang Chen, Yibao Chen, Yong Chen, Yupeng Cui, Wei Cui, Weiwei Deng, Jingkang Dong, Yongwei Du, Yuanyuan Fu, Minxue Gao, Guanhua Gao, He Gao, Min Gu, Yudong Guan, Ju Guo, Chengcheng Han, Dawei Huang, Yue Huo, Jia Jia, Shumei Jiang, Luhua Jiang, Weichun Jin, Jing Jin, Yongjie Kong, Lingda Li, Bing Li, Chengkui Li, Gang Li, Maoshun Li, Tipei Li, Wei Li, Xian Li, Xiaobo Li, Xufang Li, Yanguo Li, Zhengwei Liang, Xiaohua Liao, Jinyuan Liu, Congzhan Liu, Guoqing Liu, Hongwei Liu, Xiaojing Liu, Yinong Lu, Bo Lu, Fangjun Lu, Xuefeng Luo, Qi Luo, Tao Ma, Xiang Meng, Bin Nang, Yi Nie, Jianyin Ou, Ge Qu, Jinlu Sai, Na Shang, Rencheng Song, Liming Song, Xinying Sun, Liang Tan, Ying Tao, Lian Wang, Chen Wang, Guofeng Wang, Juan Wang, Lingjun Wang, Wenshuai Wang, Yusa Wen, Xiangyang Wu, Baiyang Wu, Bobing Wu, Mei Xiao, Guangcheng Xiao, Shuo Xiong, Shaolin Xu, Yupeng Yang, Jiawei Yang, Sheng Yang, Yanji Yi, Qibin Yin, Qianqing You, Yuan Zhang, Aimei Zhang, Chengmo Zhang, Fan Zhang, Hongmei Zhang, Juan Zhang, Tong Zhang, Wanchang Zhang, Wei Zhang, Wenzhao Zhang, Yi Zhang, Yifei Zhang, Yongjie Zhang, Yue Zhang, Zhao Zhang, Ziliang Zhao, Haisheng Zhao, Xiaofan Zheng, Shijie Zhou, Dengke Zhou, Jianfeng Zhu, Yuxuan Zhu, Yue Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 |
| title | Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 |
| title_full | Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 |
| title_fullStr | Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 |
| title_full_unstemmed | Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 |
| title_short | Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070 |
| title_sort | insight-hxmt observations of jet-like corona in a black hole x-ray binary maxi j1820+070 |
| topic | Article |
| url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7884741/ https://www.ncbi.nlm.nih.gov/pubmed/33589623 http://dx.doi.org/10.1038/s41467-021-21169-5 |
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