Zobrazeno 1 - 10
of 119
pro vyhledávání: '"Ti-Pei Li"'
Autor:
Chao Zheng, Yan-Qiu Zhang, Shao-Lin Xiong, Cheng-Kui Li, He Gao, Wang-Chen Xue, Jia-Cong Liu, Chen-Wei Wang, Wen-Jun Tan, Wen-Xi Peng, Zheng-Hua An, Ce Cai, Ming-Yu Ge, Dong-Ya Guo, Yue Huang, Bing Li, Ti-Pei Li, Xiao-Bo Li, Xin-Qiao Li, Xu-Fang Li, Jin-Yuan Liao, Cong-Zhan Liu, Fang-Jun Lu, Xiang Ma, Rui Qiao, Li-Ming Song, Jin Wang, Ping Wang, Xi-Lu Wang, Yue Wang, Xiang-Yang Wen, Shuo Xiao, Yan-Bing Xu, Yu-Peng Xu, Zhi-Guo Yao, Qi-Bing Yi, Shu-Xu Yi, Yuan You, Fan Zhang, Jin-Peng Zhang, Peng Zhang, Shu Zhang, Shuang-Nan Zhang, Yan-Ting Zhang, Zhen Zhang, Xiao-Yun Zhao, Yi Zhao, Shi-Jie Zheng
Publikováno v:
The Astrophysical Journal Letters, Vol 962, Iss 1, p L2 (2024)
The early afterglow of a gamma-ray burst (GRB) can provide critical information on the jet and progenitor of the GRB. The extreme brightness of GRB 221009A allows us to probe its early afterglow in unprecedented detail. In this Letter, we report comp
Externí odkaz:
https://doaj.org/article/9661393924584b919b41a300d6cb4c12
Autor:
Shuo Xiao, Yan-Qiu Zhang, Zi-Pei Zhu, Shao-Lin Xiong, He Gao, Dong Xu, Shuang-Nan Zhang, Wen-Xi Peng, Xiao-Bo Li, Peng Zhang, Fang-Jun Lu, Lin Lin, Liang-Duan Liu, Zhen Zhang, Ming-Yu Ge, You-Li Tuo, Wang-Chen Xue, Shao-Yu Fu, Xing Liu, Jin-Zhong Liu, An Li, Tian-Cong Wang, Chao Zheng, Yue Wang, Shuai-Qing Jiang, Jin-Da Li, Jia-Cong Liu, Zhou-Jian Cao, Xi-hong Luo, Jiao-jiao Yang, Shu-Xu Yi, Xi-Lu Wang, Ce Cai, Qi-Bin Yi, Yi Zhao, Sheng-Lun Xie, Cheng-Kui Li, Qi Luo, Li-Ming Song, Shu Zhang, Jin-Lu Qu, Cong-Zhan Liu, Xu-Fang Li, Yu-Peng Xu, Ti-Pei Li
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 1, p 6 (2024)
The milestone discovery of GW170817-GRB 170817A-AT 2017gfo has shown that gravitational waves (GWs) could be produced during the merger of a neutron star–neutron star/black hole and that in electromagnetic (EM) waves, a gamma-ray burst (GRB) and a
Externí odkaz:
https://doaj.org/article/dcc9bc6c9fd0408ea6c7cbdebf860c7b
Autor:
Wei Yu, Qing-Cui Bu, He-Xin Liu, Yue Huang, Liang Zhang, Zi-Xu Yang, Jin-Lu Qu, Shu Zhang, Li-Ming Song, Shuang-Nan Zhang, Shu-Mei Jia, Xiang Ma, Lian Tao, Ming-Yu Ge, Qing-Zhong Liu, Jing-Zhi Yan, Xue-Lei Cao, Zhi Chang, Li Chen, Yong Chen, Yu-Peng Chen, Guo-Qiang Ding, Ju Guan, Jing Jin, Ling-Da Kong, Bing Li, Cheng-Kui Li, Ti-Pei Li, Xiao-Bo Li, Jin-Yuan Liao, Bai-Sheng Liu, Cong-Zhan Liu, Fang-Jun Lu, Rui-Can Ma, Jian-Yin Nie, Xiao-Qin Ren, Na Sai, Ying Tan, You-Li Tuo, Ling-Jun Wang, Peng-Ju Wang, Bai-Yang Wu, Guang-Cheng Xiao, Qian-Qing Yin, Yuan You, Juan Zhang, Peng Zhang, Wei Zhang, Hai-Sheng Zhao, Shi-Jie Zheng, Deng-Ke Zhou
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 2, p 191 (2023)
We have performed a spectral-timing analysis of the black hole X-ray binary MAXI J1535-571 during its 2017 outburst, with the aim of exploring the evolution of the inner accretion flow geometry. X-ray reverberation lags are observed in the hard-inter
Externí odkaz:
https://doaj.org/article/e7f9b8b6e542460e93c41a354ffe84ff
Autor:
Shuo Xiao, Wen-Xi Peng, Shuang-Nan Zhang, Shao-Lin Xiong, Xiao-Bo Li, You-Li Tuo, He Gao, Yue Wang, Wang-Chen Xue, Chao Zheng, Yan-Qiu Zhang, Jia-Cong Liu, Cheng-Kui Li, Shu-Xu Yi, Xi-Lu Wang, Zhen Zhang, Ce Cai, Ai-Jun Dong, Wei Xie, Jian-Chao Feng, Qing-Bo Ma, De-Hua Wang, Xi-Hong Luo, Qi-Jun Zhi, Li-Ming Song, Ti-Pei Li
The precursors of short and long Gamma Ray Bursts (SGRBs and LGRBs) can serve as probes of their progenitors, as well as shedding light on the physical processes of mergers or core-collapse supernovae. Some models predict the possible existence of Qu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f85a3112b853831270e6927db1e1371
http://arxiv.org/abs/2210.08491
http://arxiv.org/abs/2210.08491
Autor:
Prahlad Epili, ShiJie Zheng, Yuan-Yuan Du, Peng Zhang, W. C. Jiang, Y. M. Tang, T. Luo, C. Z. Liu, S. Yang, Y. B. Chen, Xin Ren, Xufang Li, Gang Li, Cheng-Cheng Guo, Y. J. Yang, N. Sai, W. S. Wang, Wei Wang, Lei Sun, Zhe Chang, W. G. Li, X.W. Ma, L. D. Kong, Q. Luo, Bin Meng, Y. S. Wang, Jin-Yuan Liao, X. L. Cao, Da-Wei Han, Lian Tao, L. Wang, Tianran Chen, Y. G. Zheng, C. Cai, Xiong Li, Yu-Dong Gu, G. H. Gao, Mingyu Wu, Ming-Yu Ge, Y. Huang, B. Y. Wu, Weiguang Cui, Qingcui Bu, J. J. Yang, He-Yang Liu, L. Chen, Xiaohua Liang, Yuan You, X. Y. Song, R. C. Ma, Shuo Xiao, D. K. Zhou, Youli Tuo, Yi Zhang, He Gao, Jin-Lu Qu, Shaolin Xiong, Xuchao Zhao, Bing Li, Ju Guan, R. J. Yang, F. Zhang, B. B. Yi, H. M. Zhang, Jing Jin, X. F. Li, Wenda Zhang, Bobing Wu, Ti-Pei Li, Li-Ming Song, C. Wang, Junqiang Zhang, Bai-Sheng Liu, C. K. Li, Fangjun Lu, Shuang-Nan Zhang, G. C. Xiao, W. C. Zhang, Jundan Nie, Hongwei Liu, HongSheng Zhao, S. N. Zhang, Q. Q. Yin, Y. P. Chen, Y. Nang, P. J. Wang, Shu-Mei Jia, Ge Ou, Yin Xu, Jia Huo, X. Y. Wen, Z. W. Li, Xin Lu
Publikováno v:
Journal of High Energy Astrophysics. 30:1-8
GRO J1008-57, as a Be/X-ray transient pulsar, is considered to have the highest magnetic field in known neutron star X-ray binary systems. Observational data of the X-ray outbursts in GRO J1008-57 from 2017 to 2020 were collected by the Insight-HXMT
Autor:
Xiaobo Li, Zhu Liu, Y. L. Tuo, J. W. Yang, Shuang-Nan Zhang, Aimei Zhang, Yong Chen, Wei Wang, Li Chen, Mao-Shun Li, Hai-Sheng Zhao, C. K. Li, Cheng-Kui Li, Weimin Yuan, Yanji Yang, Juan Wang, Yu-Xuan Zhu, Ju Guan, Xiao-Fan Zhao, Bozena Czerny, Ling-Jun Wang, Qingwen Wu, Xufang Li, Gang Li, R. C. Shang, B. B. Wu, Shaolin Xiong, Yifei Zhang, Tong Zhang, X. Y. Song, Yongjie Zhang, N. Sai, Erlin Qiao, Yi Zhang, Ti-Pei Li, Lian Tao, Wei-Wei Cui, Wan-Chang Zhang, Bin Meng, Yue Zhu, Y. Nang, Liang Sun, Yu-Peng Chen, Ming-Yu Ge, Xiao-Jing Liu, Wei Cui, Zi-Gao Dai, Bobing Wu, Shu Zhang, Gang Chen, Bing Li, Yuan-Yuan Du, Zhi Chang, G. F. Wang, Xiang Ma, Ying Tan, L. D. Kong, T. Luo, Fangjun Lu, Guan-Hua Gao, Shuo Xiao, Juan Zhang, D. K. Zhou, Shu-Mei Jia, Y. P. Chen, Chichuan Jin, Bifang Liu, Wei Li, Jian-Feng Zhou, Ge Ou, Yupeng Xu, Bo Lu, Bei You, He Gao, Chen Wang, Fan Zhang, Yanguo Li, Chong Luo, Qi Luo, Jing Jin, Jing-Kang Deng, Li-Ming Song, Cheng-Cheng Guo, XiangYang Wen, Xiaohua Liang, C. X. Liu, C. Cai, Yue Huang, Yuan You, Jia Huo, Zi-Liang Zhang, J. C. Liu, Zhao Zhang, Yongwei Dong, Qi-Bin Yi, Mei Wu, W. C. Jiang, Jin-Yuan Liao, X. L. Cao, Xue-Feng Lu, Guang-Cheng Xiao, Wei Zhang, Chengmo Zhang, Yu-Dong Gu, Hong-Mei Zhang, Tian-Xiang Chen, GuoQing Liu, Y. N. Liu, Qian-Qing Yin, Zheng-Wei Li, Xian Li, Hongwei Liu, Sheng Yang, Wenshuai Wang, Luhua Jiang, Jin-Lu Qu, Jianyin Nie, Min-Xue Fu, Yu-Sa Wang, YongJie Jin, Yue Zhang, Qingcui Bu, Wen-Zhao Zhang, Da-Wei Han, M. Gao, Shi-Jie Zheng
Publikováno v:
Nature Communications, Vol 12, Iss 1, Pp 1-11 (2021)
Nature Communications
Nature Communications
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
Autor:
Ti-Pei Li
Publikováno v:
Space Science in China ISBN: 9780203739082
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d43c59fcc1895a35bfa12caeaecb9cc8
https://doi.org/10.1201/9780203739082-5
https://doi.org/10.1201/9780203739082-5
Autor:
Yongjie Zhang, Xian Li, Sheng Yang, Zi-Liang Zhang, Yan-Ting Dong, Lian Tao, X. Y. Song, Yupeng Xu, YongJie Jin, Ji-Ren Liu, Mei Wu, T. Luo, Jing Jin, Wan-Chang Zhang, GuoQing Liu, Chen Wang, Wei Cui, S. Xiao, XiangYang Wen, Yu-Dong Gu, Jianyin Nie, Jing-Kang Deng, Xiao-Fan Zhao, J. W. Yang, Yanji Yang, Xiaobo Li, Jia Huo, Yuan You, Gang Li, Youli Tuo, Mao-Shun Li, Qi-Bin Yi, Xufang Li, B. S. Liu, Zheng-Wei Li, Jin-Lu Qu, Yanguo Li, Xue-Ying Zheng, Yu-Peng Chen, Wei Zhang, Cheng-Cheng Guo, Yi Zhang, Li-Ming Song, Juan Zhang, N. Sai, C. Cai, Shaolin Xiong, Xue-Feng Lu, ShiJie Zheng, Jian-Feng Zhou, Q. Luo, Y. P. Chen, L. D. Kong, Wei-Wei Cui, Yongwei Dong, Yuan-Yuan Du, Bing Li, Da-Wei Han, Bin Meng, HongMei Zhang, Li-Jun Gou, Ying Tan, Zhi Zhang, C. L. Zhang, Juan Wang, D. K. Zhou, Shu Zhang, Min-Xue Fu, Jin-Yuan Liao, X. L. Cao, H. T. Liu, LuHua Jiang, Hai-Sheng Zhao, Yu-Sa Wang, X. H. Liang, Ye Feng, Yue Zhang, Guang-Cheng Xiao, Bo Lu, Qingcui Bu, Fangjun Lu, He Gao, Li Chen, Ju Guan, Yong Chen, B. B. Wu, Tong Zhang, Guan-Hua Gao, Shu-Mei Jia, W. S. Wang, Ge Ou, W. C. Jiang, Liang Sun, Tian-Xiang Chen, Qian-Qing Yin, Wei Li, Y. Nang, G. F. Wang, Xiang Ma, Yue-Zhu, Zhao Zhang, W. Z. Zhang, Nan Jia, Fan Zhang, Yu-Xuan Zhu, Yifei Zhang, Shuang-Nan Zhang, Aimei Zhang, Ming-Yu Ge, Xiao-Jing Liu, Yu-Feng Li, Yue Huang, R. C. Shang, Zhi Chang, Zhen-Xuan Liao, H. W. Liu, Gang Chen, Cheng-Kui Li, Yi-Rong Yang, Y. N. Liu, Bobing Wu, Ti-Pei Li, M. Gao, Xue-Shan Zhao, R. L. Zhuang, C. X. Liu
Publikováno v:
Journal of High Energy Astrophysics. 27:53-63
Recently, the system parameters of Cygnus X-1, i.e., the black hole mass M, the orbital inclination i and the source distance D, have been updated. As the input constraints of the continuum-fitting method, it is necessary to refine the spin with thes
Autor:
Z. W. Li, Jin-Lu Qu, He Gao, Y. C. Zhu, Xin Lu, J. X. Wang, ShaoZhen Liu, S. Yang, Xufang Li, Z. Zhang, Z. L. Zhang, Gang Li, W. C. Zhang, Yan Zhu, Long Ji, N. Sai, F. Zhang, Wenda Zhang, Bin Meng, Y. Tan, W. C. Jiang, Chuan-Peng Zhang, He-Yang Liu, Guo-Ming Chen, ShiJie Zheng, Bobing Wu, Y. G. Zheng, C. Cai, J. F. Zhou, D. K. Zhou, T. Luo, Ti-Pei Li, Shuo Xiao, Yuan-Yuan Du, Zhe Chang, Y. N. Liu, X.W. Ma, Tianran Chen, Shu-Mei Jia, Yu-Dong Gu, Bo Lu, Mingyu Wu, Lian Tao, Bing Li, Xuchao Zhao, Jing Jin, Jia Huo, X. Y. Wen, Ju Guan, Fangjun Lu, Jundan Nie, Ge Ou, X. F. Li, Cheng-Cheng Guo, M. Gao, Lei Sun, Hongwei Liu, Y. G. Li, C. Z. Liu, Luhua Jiang, H. M. Zhang, C. Wang, W. S. Wang, W. Z. Zhang, W. G. Li, He Xu, G. H. Gao, Jin-Yuan Liao, X. L. Cao, Min-Xue Fu, Shaolin Xiong, Y. Nang, Y. S. Wang, Junqiang Zhang, Mingzhe Li, Jinyi Yang, Y. Zhang, C. K. Li, Y. Huang, GuoQing Liu, P. J. Wang, Youcai Zhang, Jing-Kang Deng, Xiaohua Liang, G. F. Wang, Yi Zhang, Yuan You, Youli Tuo, Xin Ren, Yin Xu, Weiguang Cui, Q. Luo, Qingcui Bu, L. D. Kong, Y. B. Chen, Ming-Yu Ge, Xiao-Jing Liu, Da-Wei Han, Shuang-Nan Zhang, Li-Ming Song, Wei-Wei Cui, Aimei Zhang, Shuinai Zhang, Peng Zhang, Y. W. Dong, G. C. Xiao, HongSheng Zhao, Y. P. Chen, Xiaobo Li, L. Chen, Yi-Yan Yang, X. Y. Song, Y. J. Yang, T. Zhang, Q. B. Yi, B. Y. Wu
Publikováno v:
Journal of High Energy Astrophysics. 25:29-38
A new black hole X-ray binary (BHXRB) MAXI J1535-571 was discovered by MAXI during its outburst in 2017. Using observations taken by the first Chinese X-ray satellite, the Hard X-ray Modulation Telescope (dubbed as Insight-HXMT), we perform a joint s
Autor:
Jing-Kang Deng, Shaolin Xiong, Q. Luo, Xiaohua Liang, Yuan You, Youli Tuo, Jing Jin, Yin Xu, Jinyi Yang, X. F. Li, Z. L. Zhang, Ju Guan, Y. B. Chen, Lei Sun, Fangjun Lu, Da-Wei Han, Mingzhe Li, W. G. Li, Wenda Zhang, C. Cai, Chuan-Peng Zhang, Y. Huang, Z. W. Li, Jundan Nie, Can Güngör, Hongwei Liu, Li-Ming Song, Y. G. Li, Bobing Wu, Andrea Santangelo, Xufang Li, ShiJie Zheng, Min-Xue Fu, Luhua Jiang, Ti-Pei Li, Gang Li, Y. W. Dong, N. Sai, J. X. Wang, Y. Nang, G. C. Xiao, Shuinai Zhang, Jing Zhou, Xin Lu, Y. N. Liu, Yuan-Yuan Du, Jia Huo, X. Y. Wen, Junqiang Zhang, Y. Tan, F. Zhang, Bin Meng, W. C. Jiang, G. F. Wang, Yi Zhang, C. K. Li, Wei-Wei Cui, L. D. Kong, H. M. Zhang, Shuo Xiao, W. C. Zhang, M. Gao, Bo Lu, Guo-Ming Chen, Xuchao Zhao, C. Wang, Shu-Mei Jia, Shuang-Nan Zhang, G. H. Gao, Aimei Zhang, Ge Ou, Weiguang Cui, Qingcui Bu, HongSheng Zhao, C. Z. Liu, W. Z. Zhang, Y. Zhang, Mingyu Wu, Q. Q. Yin, Y. P. Chen, GuoQing Liu, Bing Li, Y. J. Yang, D. K. Zhou, Y. S. Wang, Yi Chen, Ming-Yu Ge, Xiao-Jing Liu, Xiaobo Li, Youcai Zhang, S. Yang, L. Chen, X. Y. Song, Zhe Chang, T. Zhang, X.W. Ma, Lian Tao, Yi-Nan Zhu, Cheng-Cheng Guo, W. S. Wang, T. Luo, Q. B. Yi, B. Y. Wu, Jin-Yuan Liao, X. L. Cao, He Gao, Z. Zhang, Yan Zhu, Long Ji, Tianran Chen, Yu-Dong Gu
Publikováno v:
Journal of High Energy Astrophysics. 25:10-16
We study the 2018 outburst of Aql X-1 via the monitor of all sky X-ray image (MAXI) data. We show that the outburst starting in February 2018 is a member of short-low class in the frame of outburst duration and the peak count rate although the outbur