Zobrazeno 1 - 10
of 979
pro vyhledávání: '"Jing, Qiang"'
Autor:
Shui, Qing-Cang, Zhang, Shu, Peng, Jing-Qiang, Zhang, Shuang-Nan, Chen, Yu-Peng, Kong, Ling-Da, Yu, Zhuo-Li, Ji, Long, Wang, Peng-Ju, Chang, Zhi, Yin, Hong-Xing, Li, Jian
IGR J17091-3624, in addition to GRS 1915+105, is the only black hole X-ray binary that displays ``heartbeat"-like variability characterized by structured flares with high amplitudes. In this study, we conduct a detailed phase-resolved analysis of the
Externí odkaz:
http://arxiv.org/abs/2407.19388
Autor:
Duan, Qing-Chen, Liu, Shao-Hua, Li, Bai-Zhuo, Meng, Jiao-Jiao, Yang, Wu-Zhang, Liu, Yi, Lin, Yi-Qiang, Wu, Si-Qi, Lu, Jia-Yi, Bao, Jin-Ke, Xiao, Yu-Sen, Zhao, Xin-Yu, Mei, Yu-Xue, Sun, Yu-Ping, Yu, Dan, Tan, Shu-Gang, Jing, Qiang, Zhong, Rui-Dan, Chen, Yong-Liang, Zhao, Yong, Ren, Zhi, Wang, Cao, Cao, Guang-Han
We report the synthesis, crystal structure, and physical properties of a novel ternary compound, Th$_2$Cu$_4$As$_5$. The material crystallizes in a tetragonal structure with lattice parameters $a=4.0716(1)$ {\AA} and $c=24.8131(4)$ {\AA}. Its structu
Externí odkaz:
http://arxiv.org/abs/2311.13308
Autor:
An, Zheng-Hua, Antier, S., Bi, Xing-Zi, Bu, Qing-Cui, Cai, Ce, Cao, Xue-Lei, Camisasca, Anna-Elisa, Chang, Zhi, Chen, Gang, Chen, Li, Chen, Tian-Xiang, Chen, Wen, Chen, Yi-Bao, Chen, Yong, Chen, Yu-Peng, Coughlin, Michael W., Cui, Wei-Wei, Dai, Zi-Gao, Hussenot-Desenonges, T., Du, Yan-Qi, Du, Yuan-Yuan, Du, Yun-Fei, Fan, Cheng-Cheng, Frontera, Filippo, Gao, He, Gao, Min, Ge, Ming-Yu, Gong, Ke, Gu, Yu-Dong, Guan, Ju, Guo, Dong-Ya, Guo, Zhi-Wei, Guidorzi, Cristiano, Han, Da-Wei, He, Jian-Jian, He, Jun-Wang, Hou, Dong-Jie, Huang, Yue, Huo, Jia, Ji, Zhen, Jia, Shu-Mei, Jiang, Wei-Chun, Kann, David Alexander, Klotz, A., Kong, Ling-Da, Lan, Lin, Li, An, Li, Bing, Li, Chao-Yang, Li, Cheng-Kui, Li, Gang, Li, Mao-Shun, Li, Ti-Pei, Li, Wei, Li, Xiao-Bo, Li, Xin-Qiao, Li, Xu-Fang, Li, Yan-Guo, Li, Zheng-Wei, Liang, Jing, Liang, Xiao-Hua, Liao, Jin-Yuan, Lin, Lin, Liu, Cong-Zhan, Liu, He-Xin, Liu, Hong-Wei, Liu, Jia-Cong, Liu, Xiao-Jing, Liu, Ya-Qing, Liu, Yu-Rong, Lu, Fang-Jun, Lu, Hong, Lu, Xue-Feng, Luo, Qi, Luo, Tao, Ma, Bin-Yuan, Ma, Fu-Li, Ma, Rui-Can, Ma, Xiang, Maccary, Romain, Mao, Ji-Rong, Meng, Bin, Nie, Jian-Yin, Orlandini, Mauro, Ou, Ge, Peng, Jing-Qiang, Peng, Wen-Xi, Qiao, Rui, Qu, Jin-Lu, Ren, Xiao-Qin, Shi, Jing-Yan, Shi, Qi, Song, Li-Ming, Song, Xin-Ying, Su, Ju, Sun, Gong-Xing, Sun, Liang, Sun, Xi-Lei, Tan, Wen-Jun, Tan, Ying, Tao, Lian, Tuo, You-Li, Turpin, Damien, Wang, Jin-Zhou, Wang, Chen, Wang, Chen-Wei, Wang, Hong-Jun, Wang, Hui, Wang, Jin, Wang, Ling-Jun, Wang, Peng-Ju, Wang, Ping, Wang, Wen-Shuai, Wang, Xiang-Yu, Wang, Xi-Lu, Wang, Yu-Sa, Wang, Yue, Wen, Xiang-Yang, Wu, Bo-Bing, Wu, Bai-Yang, Wu, Hong, Xiao, Sheng-Hui, Xiao, Shuo, Xiao, Yun-Xiang, Xie, Sheng-Lun, Xiong, Shao-Lin, Xiong, Sen-Lin, Xu, Dong, Xu, He, Xu, Yan-Jun, Xu, Yan-Bing, Xu, Ying-Chen, Xu, Yu-Peng, Xue, Wang-Chen, Yang, Sheng, Yang, Yan-Ji, Yang, Zi-Xu, Ye, Wen-Tao, Yi, Qi-Bin, Yi, Shu-Xu, Yin, Qian-Qing, You, Yuan, Yu, Yun-Wei, Yu, Wei, Yu, Wen-Hui, Zeng, Ming, Zhang, Bing, Zhang, Bin-Bin, Zhang, Da-Li, Zhang, Fan, Zhang, Hong-Mei, Zhang, Juan, Zhang, Liang, Zhang, Peng, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Wan-Chang, Zhang, Xiao-Feng, Zhang, Xiao-Lu, Zhang, Yan-Qiu, Zhang, Yan-Ting, Zhang, Yi-Fei, Zhang, Yuan-Hang, Zhang, Zhen, Zhao, Guo-Ying, Zhao, Hai-Sheng, Zhao, Hong-Yu, Zhao, Qing-Xia, Zhao, Shu-Jie, Zhao, Xiao-Yun, Zhao, Xiao-Fan, Zhao, Yi, Zheng, Chao, Zheng, Shi-Jie, Zhou, Deng-Ke, Zhou, Xing, Zhu, Xiao-Cheng
GRB 221009A is the brightest gamma-ray burst ever detected since the discovery of this kind of energetic explosions. However, an accurate measurement of the prompt emission properties of this burst is very challenging due to its exceptional brightnes
Externí odkaz:
http://arxiv.org/abs/2303.01203
Autor:
Shui, Qing-Cang, Zhang, Shu, Chen, Yu-Peng P., Zhang, Shuang-Nan, Kong, Ling-Da, Wang, Peng-Ju, Ji, Long, Yin, Hong-Xing, Qu, J. L., Tao, L., Ge, M. Y., Peng, Jing-Qiang, Chang, Zhi, Li, Jian, Zhang, Peng
We present a systematic analysis of type C quasi-periodic oscillation (QPO) observations of H 1743--322 throughout the Rossi X-ray Timing Explorer (RXTE) era. We find that, while different outbursts have significant flux differences, they show consis
Externí odkaz:
http://arxiv.org/abs/2211.16679
Autor:
Chen, Yu-Peng, Zhang, Shu, Zhang, Shuang-Nan, Ji, Long, Wang, Peng-Ju, Kong, Ling-Da, Chang, Zhi, Peng, Jing-Qiang, Shui, Qing-Cang, Li, Jian, Tao, Lian, Ge, Ming-Yu, Qu, Jin-Lu
After in quiescence for 49 years, 4U~1730--22 became active and had two outbursts in 2021 \& 2022, the onset and tail of the outbursts were observed by NICER, which give us a peerless opportunity to study the state transition and its underlying mecha
Externí odkaz:
http://arxiv.org/abs/2211.10160
Autor:
Chen, Yu-Peng, Zhang, Shu, Ji, Long, Zhang, Shuang-Nan, Kong, Ling-Da, Wang, Peng-Ju, Chang, Zhi, Peng, Jing-Qiang, Li, Jian, Qu, Jin-Lu, Li, Zhao-Sheng, Tao, Lian, Ge, Ming-Yu
After in quiescence for 49 years, 4U~1730--22 became active and had two outbursts in 2021 \& 2022; ten thermonuclear X-ray bursts were detected with Insight-HXMT. Among them, the faintest burst showed a double-peaked profile, placing the source as th
Externí odkaz:
http://arxiv.org/abs/2209.10721
Autor:
Chen, Yu-Peng, Zhang, Shu, Ji, Long, Zhang, Shuang-Nan, Kong, Ling-Da, Wang, Peng-Ju, Chang, Zhi, Peng, Jing-Qiang, Li, Jian, Qu, Jin-Lu
A type-I burst could influence the accretion process through radiation pressure and Comptonization both for the accretion disk and the corona/boundary layer of an X-ray binary, and vice versa. We investigate the temporal evolution of a bright photosp
Externí odkaz:
http://arxiv.org/abs/2208.13556
Autor:
Yu-Peng, Chen, Shu, Zhang, Long, Ji, Shuang-Nan, Zhang, Peng-Ju, Wang, Ling-Da, Kong, Zhi, Chang, Jing-Qiang, Peng, Qing-Cang, Shui, Jian, Li, Lian, Tao, Ming-Yu, Ge, Jin-Lu, Qu
MAXI J1816-195 is a newly discovered accreting millisecond pulsar with prolific thermonuclear bursts, detected during its outburst in 2022 June by Insight-HXMT and NICER. During the outburst, Insight-HXMT detected 73 bursts in its peak and decay phas
Externí odkaz:
http://arxiv.org/abs/2208.12124
Autor:
Kong, Ling-Da, Zhang, Shu, Zhang, Shuang-Nan, Ji, Long, Doroshenko, Victor, Santangelo, Andrea, Chen, Yu-Peng, Lu, Fang-Jun, Ge, Ming-Yu, Wang, Peng-Ju, Tao, Lian, Qu, Jin-Lu, Li, Ti-Pei, Liu, Cong-Zhan, Liao, Jin-Yuan, Chang, Zhi, Peng, Jing-Qiang, Shui, Qing-Cang
The detection of cyclotron resonance scattering features (CRSFs) is the only way to directly and reliably measure the magnetic field near the surface of a neutron star (NS). The broad energy coverage and large collection area of \emph{Insight}-HXMT i
Externí odkaz:
http://arxiv.org/abs/2206.04283
Publikováno v:
In Materials Today Sustainability September 2024 27