Ultrahigh-energy gamma-ray emission associated with black hole-jet systems.

Black holes (BHs), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass BHs drive relativistic jets when accreting matter from their companion stars, forming microquasars. Non-thermal emission from the radio to teraelectronvolt gamma-ray band has been observed from microquasars, indicating the acceleration of relativistic particles. Here we report detection of four microquasars (SS 433, V4641 Sgr, GRS 1915+105, MAXI J1820+070) of spectra extending to the ultrahigh-energy (UHE; photon energy [Formula: see text] TeV) band, and one microquasar (Cygnus X-1) with a spectrum approaching 100 TeV, using the Large High Altitude Air Shower Observatory. Notably, the total emission associated with SS 433 cannot be interpreted with a single leptonic component. In the UHE band, its emission is in spatial coincidence with a giant atomic cloud, which is consistent with a hadronic origin. An elongated source is discovered from V4641 Sgr with the spectrum continuing up to 800 TeV. The detection of UHE gamma rays demonstrates that accreting BHs and their environments can operate as extremely efficient accelerators of particles up to 1 PeV, suggesting that microquasars are important contributors to Galactic cosmic rays, especially around the 'knee' region.

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Publication Details

Journal
PubMed
Published
2025-12-01
DOI
https://doi.org/10.1093/nsr/nwaf496
Citations
8
Primary Topic
Astrophysics and Cosmic Phenomena
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article
Field-Weighted Citation Impact
14.96

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article

Ultrahigh-energy gamma-ray emission associated with black hole-jet systems.

S D Li, Xiaoyuan Huang, Ling‐Yu Wang, Hengyun Zhang et al.
8 citations
PubMed
Astrophysics and Cosmic Phenomena
14.96
article

Ultrahigh-energy gamma-ray emission associated with black hole-jet systems.

S D Li, Xiaoyuan Huang, Ling‐Yu Wang, Hengyun Zhang, B. S. Gao, Yao Huang, O. Shchegolev, Dongyang Liu, H X Chen, R. Wang, Chufan Cai, Yiliang Xin, Lili Yang, Lu‐Yang Wang, Y. W. Bao, Y. D. Wang, J. Liu, Yi-Zhong Fan, Yaodong Cheng, P P Zhang, Q. N. Sun, Z. G. Yao, Yalan Xing, Ruixi Li, Haigang Wang, Ping Zhou, J. Guo, Mi Zhou, K. J. Zhu, J R Liu, Bingyan Liu, H B Li, H.K Lv, T. Y. Li, Chengyuan Wu, Kenny C. Y. Ng, Jiang‐Ning Zhou, Yujiang Bi, J. L. Zhang, Z.X. Wang, En‐Wei Liang, Yi-Qing Guo, Ali Raza, Y. Feng, X. T. Hou, Renxin Xu, G. Gong, Qi Gao, D. L. Xu, Yudong Cui, Mengyuan Qi, Z. J. Jiang, Ke Wang, M. M. Ge, H. C. Song, Yang Shen, A. Neronov, Tianyu Ge, D. Kuleshov, Z. Y. Pei, Li‐Sheng Geng, Xing‐Xiang He, Sha Sha Wu, Xiaohong Cui, Hongwei Mu, H. Y. Jia, Weiya Zhang, C. F. Feng, Y N Liu, Weiwei Cao, Kai Li, F Aharonian, Haixia Jiang, Zhebin Sun, D. Semikoz, Dahai Yan, S H Chen, Yuzhen Feng, J. F. Chang, X P Zhang, G W Wang, Z. Cao, F Zhang, Michael Y. Ni, Weixin Bian, Yong Guo, Rongfu Xu, Guobin Mou, X J Chen, Hancheng Li, Long Zhao, Jianying He, Chuyuan Yang, Xu Guo, Y. Chen, Da-Ming Wei, Renquan Yang, J. Takata, W. Mitthumsiri, S Z Chen, Shuai Feng, Yujie Wei, H. L. Dai, N Yin, Fulai Guo, Shan Zhang, Q. Luo, Yun-Feng Liang, H Feng, Teng Huang, Shengyong Chen, Yu. V. Stenkin, Bin Zhou, Fa‐Kun Zheng, Ryan W. Tang, Dingrong Xiong, P F Zhang, Youwu Su, Ming Jin, B Z Dai, Jing Huang, M. C. Chu, Fengchun Shu, Ke Fang, X. H. You, D. Ruffolo, Hongming Zhu, Qing-Wen Tang, B Q, Bingbing Li, Jin Chang, Jing Xia, H D Liu, Gwenael Giacinti, Z H Wang, Y Z Li, W. J. Huang, Jianglai Liu, Fan Yang, H. H. He, Yangmin Diao, Qi Chen, Z. Tang, Sheng Hu, M. Zahid Hasan, Q. B. Gou, X. N. Sun, Jiyong Zhao, Xungai Wang, X. D. Sheng, Cunzhu Tong, Zi-Gao Dai, A. Sáiz, Cuilan Ren, K. Jia, K. Kurinov, L. Shao, Xuefeng Jiang, Shoushan Zhang, Jing‐Zhi Yan, O. A. Hannuksela, W Liu, Shaoyang Zhao, Chen Huang, T. L. Chen, Yunfeng Luo, Y. Huang, X B Chen, M L Chen, V. Stepanov, Feifei Yang, S. Hernández-Cadena, Chul Woo Yang, Jun Fang, A.V Bukevich, Xinhua Ma, Yi Liu, Hongjun Zhang, Cong Li, Liang Chen, Long Chen, Xin Li, Zhe Li, Yi Wang, Chun Wang, Xiaoyan Wang, Wei Wang, Jian Li, Y. Bai, Rui Zhang, Li Zhang, Jie Li, Kai You Wang, Kai Wang, Lei Li, Hongming Zhang, Di Li, Zhuo Li, Xia‐Ting Feng, Xiaohan Li, Yinong Liu, Yong‐Wei Zhang, Hao Sun, Min Yang, Michael Chen, Guohua Chen, Li‐Sheng Wang, Boyu Zhang, Ruo-Yu Liu, Bin‐Bin Zhang, Rong Zhou, Y. Li, Li Fei, Xingjun Wang, Feng Liu, Z. Zhang, Weilong Li, Haichao Liu, Xinhua Zhou, Xiaoxia Wu, Haoning He, Allen Chen, Mingyue Cui, Baohua Zhu, S. W. Cui, Wenlong Gao, Jingjing Wei, X. X. Zhou, Hui‐Yi Zeng, Haiyan Tan, Junjie Qin, X. Zhang, Zhuofan Shi, Y.‐Q. Lou, J. Fang, Na Cheng, Yi Zhang, L. Q. Yin, C. Hou, Xiaohong Zhao, Z. Y. You, Y. A. Han, Liping Nie, M. H. Gu, K. Jiang, X. L. Ji, L.Z. Zhao, Kai-Kai Duan, T Yan, Zhe Cao, X.Q Dong, H. R. Wu, W. L. Xu, D. Bastieri, M M Kang, I. Karpikov, P. H. T. Tam, N. Zhou, Qingwen Wu, W Zeng, D. Khangulyan, W. W. Tian, D. Liu, L.L. Ma, Z. Min, X. J. Bi, Elizabeth Chen, M. Y. Liu, J.R Mao, D. Huang, Xu Ye, S Kaci, L.H Wan, Jian Chen Qi, H. B. Hu, X. T. Huang, Cuiping Liu, Y. C. Zou, S. Gabici, B. W. Hou, Chuyue Gao, P. Pattarakijwanich, T. X. Zeng, S.J Lin, Jincheng Wang, Daxi Sun, Siming Liu, X. Liu, Ting Wen, Danzengluobu Danzengluobu, Di-Xuan Xiao, Shao-Qiang Xi, Weixian Yang, L.J Ou, C. Zhang, Y. H. Yu, Yu He, C. G. Zhu, N.H Tabasam, C. Li
article en
8 citations

Abstract

Black holes (BHs), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass BHs drive relativistic jets when accreting matter from their companion stars, forming microquasars. Non-thermal emission from the radio to teraelectronvolt gamma-ray band has been observed from microquasars, indicating the acceleration of relativistic particles. Here we report detection of four microquasars (SS 433, V4641 Sgr, GRS 1915+105, MAXI J1820+070) of spectra extending to the ultrahigh-energy (UHE; photon energy [Formula: see text] TeV) band, and one microquasar (Cygnus X-1) with a spectrum approaching 100 TeV, using the Large High Altitude Air Shower Observatory. Notably, the total emission associated with SS 433 cannot be interpreted with a single leptonic component. In the UHE band, its emission is in spatial coincidence with a giant atomic cloud, which is consistent with a hadronic origin. An elongated source is discovered from V4641 Sgr with the spectrum continuing up to 800 TeV. The detection of UHE gamma rays demonstrates that accreting BHs and their environments can operate as extremely efficient accelerators of particles up to 1 PeV, suggesting that microquasars are important contributors to Galactic cosmic rays, especially around the 'knee' region.

PubMedVol. 12(12)
University of Science and Technology of China (CN), Centre National de la Recherche Scientifique (FR), Ministry of Education of the People's Republic of China (CN), Tibet University (CN), Nanchang University (CN), Guangxi University (CN), Nanjing Normal University (CN), Moscow Institute of Physics and Technology (RU), Shandong University (CN), Sun Yat-sen University (CN), Délégation Paris 7 (FR), Chinese University of Hong Kong (HK), Shanghai Jiao Tong University (CN), Yunnan University (CN), Yerevan State University (AM), Chinese Academy of Sciences (CN), Université Paris Cité (FR), Sichuan University (CN), Mahidol University (TH), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Shanghai Astronomical Observatory (CN), Observatoire de Paris (FR), Yunnan Observatories (CN), Purple Mountain Observatory (CN), Guangdong Polytechnic of Science and Technology (CN), Guangzhou University (CN), Zhengzhou University (CN), Institute for Nuclear Research (RU), Kavli Institute for Theoretical Sciences (CN), Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) (CN), National Space Science Center (CN), Zhejiang Lab (CN), Institute of High Energy Physics (CN), Max Planck Institute for Nuclear Physics (DE), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), Zhuhai Institute of Advanced Technology (CN), Institut de Recherche sur les Lois Fondamentales de l'Univers (FR), Huazhong University of Science and Technology (CN), Southwest Jiaotong University (CN), China Center of Advanced Science and Technology (CN), Nanjing University (CN), Hebei Normal University (CN), Tsinghua University (CN)
National Natural Science Foundation of China, Chinese Academy of Sciences, National Science and Technology Development Agency, National Research Council of Thailand, Department of Science and Technology of Sichuan Province, High Energy Physics
Openalex Percentile: Top 1%
Astrophysics and Cosmic Phenomena
14.96
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