Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Shen, Rongfeng"'
Autor:
Li, En-Kun, Liu, Shuai, Torres-Orjuela, Alejandro, Chen, Xian, Inayoshi, Kohei, Wang, Long, Hu, Yi-Ming, Amaro-Seoane, Pau, Askar, Abbas, Bambi, Cosimo, Capelo, Pedro R., Chen, Hong-Yu, Chua, Alvin J. K., Condés-Breña, Enrique, Dai, Lixin, Das, Debtroy, Derdzinski, Andrea, Fan, Hui-Min, Fujii, Michiko, Gao, Jie, Garg, Mudit, Ge, Hongwei, Giersz, Mirek, Huang, Shun-Jia, Hypki, Arkadiusz, Liang, Zheng-Cheng, Liu, Bin, Liu, Dongdong, Liu, Miaoxin, Liu, Yunqi, Mayer, Lucio, Napolitano, Nicola R., Peng, Peng, Shao, Yong, Shashank, Swarnim, Shen, Rongfeng, Tagawa, Hiromichi, Tanikawa, Ataru, Toscani, Martina, Vázquez-Aceves, Verónica, Wang, Hai-Tian, Yi, Shu-Xu, Zhang, Jian-dong, Zhang, Xue-Ting, Zhu, Lianggui, Zwick, Lorenz, Huang, Song, Mei, Jianwei, Wang, Yan, Xie, Yi, Zhang, Jiajun, Luo, Jun
The opening of the gravitational wave window has significantly enhanced our capacity to explore the universe's most extreme and dynamic sector. In the mHz frequency range, a diverse range of compact objects, from the most massive black holes at the f
Externí odkaz:
http://arxiv.org/abs/2409.19665
Autor:
Guo, Hengxiao, Sun, Jingbo, Li, Shuang-Liang, Jiang, Yan-Fei, Wang, Tinggui, Bu, Defu, Jiang, Ning, Wang, Yanan, Yao, Yuhan, Shen, Rongfeng, Gu, Minfeng, Sun, Mouyuan
When a star passes through the tidal disruption radius of a massive black hole (BH), it can be torn apart by the tidal force of the BH, known as the Tidal Disruption Event (TDE). Since the UV/optical emitting region inferred from the blackbody radius
Externí odkaz:
http://arxiv.org/abs/2312.06771
Autor:
Wang, Yanan, Baldi, Ranieri D., del Palacio, Santiago, Guolo, Muryel, Yang, Xiaolong, Zhang, Yangkang, Done, Chris, Segura, Noel Castro, Pasham, Dheeraj R., Middleton, Matthew, Altamirano, Diego, Gandhi, Poshak, Qiao, Erlin, Jiang, Ning, Yan, Hongliang, Giroletti, Marcello, Migliori, Giulia, McHardy, Ian, Panessa, Francesca, Jin, Chichuan, Shen, Rongfeng, Dai, Lixin
AT 2019avd is a nuclear transient detected from infrared to soft X-rays, though its nature is yet unclear. The source has shown two consecutive flaring episodes in the optical and the infrared bands and its second flare was covered by X-ray monitorin
Externí odkaz:
http://arxiv.org/abs/2212.08453
Autor:
Ge, Jian, Zhang, Hui, Zang, Weicheng, Deng, Hongping, Mao, Shude, Xie, Ji-Wei, Liu, Hui-Gen, Zhou, Ji-Lin, Willis, Kevin, Huang, Chelsea, Howell, Steve B., Feng, Fabo, Zhu, Jiapeng, Yao, Xinyu, Liu, Beibei, Aizawa, Masataka, Zhu, Wei, Li, Ya-Ping, Ma, Bo, Ye, Quanzhi, Yu, Jie, Xiang, Maosheng, Yu, Cong, Liu, Shangfei, Yang, Ming, Wang, Mu-Tian, Shi, Xian, Fang, Tong, Zong, Weikai, Liu, Jinzhong, Zhang, Yu, Zhang, Liyun, El-Badry, Kareem, Shen, Rongfeng, Tam, Pak-Hin Thomas, Hu, Zhecheng, Yang, Yanlv, Zou, Yuan-Chuan, Wu, Jia-Li, Lei, Wei-Hua, Wei, Jun-Jie, Wu, Xue-Feng, Sun, Tian-Rui, Wang, Fa-Yin, Zhang, Bin-Bin, Xu, Dong, Yang, Yuan-Pei, Li, Wen-Xiong, Xiang, Dan-Feng, Wang, Xiaofeng, Wang, Tinggui, Zhang, Bing, Jia, Peng, Yuan, Haibo, Zhang, Jinghua, Wang, Sharon Xuesong, Gan, Tianjun, Wang, Wei, Zhao, Yinan, Liu, Yujuan, Wei, Chuanxin, Kang, Yanwu, Yang, Baoyu, Qi, Chao, Liu, Xiaohua, Zhang, Quan, Zhu, Yuji, Zhou, Dan, Zhang, Congcong, Yu, Yong, Zhang, Yongshuai, Li, Yan, Tang, Zhenghong, Wang, Chaoyan, Wang, Fengtao, Li, Wei, Cheng, Pengfei, Shen, Chao, Li, Baopeng, Pan, Yue, Yang, Sen, Gao, Wei, Song, Zongxi, Wang, Jian, Zhang, Hongfei, Chen, Cheng, Wang, Hui, Zhang, Jun, Wang, Zhiyue, Zeng, Feng, Zheng, Zhenhao, Zhu, Jie, Guo, Yingfan, Zhang, Yihao, Li, Yudong, Wen, Lin, Feng, Jie, Chen, Wen, Chen, Kun, Han, Xingbo, Yang, Yingquan, Wang, Haoyu, Duan, Xuliang, Huang, Jiangjiang, Liang, Hong, Bi, Shaolan, Gai, Ning, Ge, Zhishuai, Guo, Zhao, Huang, Yang, Li, Gang, Li, Haining, Li, Tanda, Yuxi, Lu, Rix, Hans-Walter, Shi, Jianrong, Song, Fen, Tang, Yanke, Ting, Yuan-Sen, Wu, Tao, Wu, Yaqian, Yang, Taozhi, Yin, Qing-Zhu, Gould, Andrew, Lee, Chung-Uk, Dong, Subo, Yee, Jennifer C., Shvartzvald, Yossi, Yang, Hongjing, Kuang, Renkun, Zhang, Jiyuan, Liao, Shilong, Qi, Zhaoxiang, Yang, Jun, Zhang, Ruisheng, Jiang, Chen, Ou, Jian-Wen, Li, Yaguang, Beck, Paul, Bedding, Timothy R., Campante, Tiago L., Chaplin, William J., Christensen-Dalsgaard, Jørgen, García, Rafael A., Gaulme, Patrick, Gizon, Laurent, Hekker, Saskia, Huber, Daniel, Khanna, Shourya, Mathur, Savita, Miglio, Andrea, Mosser, Benoît, Ong, J. M. Joel, Santos, Ângela R. G., Stello, Dennis, Bowman, Dominic M., Lares-Martiz, Mariel, Murphy, Simon, Niu, Jia-Shu, Ma, Xiao-Yu, Molnár, László, Fu, Jian-Ning, De Cat, Peter, Su, Jie, consortium, the ET
We propose to develop a wide-field and ultra-high-precision photometric survey mission, temporarily named "Earth 2.0 (ET)". This mission is designed to measure, for the first time, the occurrence rate and the orbital distributions of Earth-sized plan
Externí odkaz:
http://arxiv.org/abs/2206.06693
Autor:
Shu, Xinwen, Zhang, Wenjie, Li, Shuo, Jiang, Ning, Dou, Liming, Yan, Zhen, Xie, Fu-Guo, Shen, Rongfeng, Sun, Luming, Liu, Fukun, Wang, Tinggui
Publikováno v:
Nat. Commun., 2020, 11, 5876
Optical transient surveys have led to the discovery of dozens of stellar tidal disruption events (TDEs) by massive black hole in the centers of galaxies. Despite extensive searches, X-ray follow-up observations have produced no or only weak X-ray det
Externí odkaz:
http://arxiv.org/abs/2012.11818
Autor:
Liu, Jifeng, Zhang, Haotong, Howard, Andrew W., Bai, Zhongrui, Lu, Youjun, Soria, Roberto, Justham, Stephen, Li, Xiangdong, Zheng, Zheng, Wang, Tinggui, Belczynski, Krzysztof, Casares, Jorge, Zhang, Wei, Yuan, Hailong, Dong, Yiqiao, Lei, Yajuan, Isaacson, Howard, Wang, Song, Bai, Yu, Shao, Yong, Gao, Qing, Wang, Yilun, Niu, Zexi, Cui, Kaiming, Zheng, Chuanjie, Mu, Xiaoyong, Zhang, Lan, Wang, Wei, Heger, Alexander, Qi, Zhaoxiang, Liao, Shilong, Lattanzi, Mario, Gu, Wei-Min, Wang, Junfeng, Wu, Jianfeng, Shao, Lijing, Shen, Rongfeng, Wang, Xiaofeng, Bregman, Joel, Di Stefano, Rosanne, Liu, Qingzhong, Han, Zhanwen, Zhang, Tianmeng, Wang, Huijuan, Ren, Juanjuan, Zhang, Junbo, Zhang, Jujia, Wang, Xiaoli, Cabrera-Lavers, Antonio, Corradi, Romano, Rebolo, Rafael, Zhao, Yongheng, Zhao, Gang, Chu, Yaoquan, Cui, Xiangqun
Publikováno v:
Nature, 575, 618-621 (2019)
All stellar mass black holes have hitherto been identified by X-rays emitted by gas that is accreting onto the black hole from a companion star. These systems are all binaries with black holes below 30 M$_{\odot}$$^{1-4}$. Theory predicts, however, t
Externí odkaz:
http://arxiv.org/abs/1911.11989
Autor:
Wen, Jiaxing, Long, Xiangyun, Zheng, Xutao, An, Yu, Cai, Zhengyang, Cang, Jirong, Che, Yuepeng, Chen, Changyu, Chen, Liangjun, Chen, Qianjun, Chen, Ziyun, Cheng, Yingjie, Deng, Litao, Deng, Wei, Ding, Wenqing, Du, Hangci, Duan, Lian, Gan, Quan, Gao, Tai, Gao, Zhiying, Han, Wenbin, Han, Yiying, He, Xinbo, He, Xinhao, Hou, Long, Hu, Fan, Hu, Junling, Huang, Bo, Huang, Dongyang, Huang, Xuefeng, Jia, Shihai, Jiang, Yuchen, Jin, Yifei, Li, Ke, Li, Siyao, Li, Yurong, Liang, Jianwei, Liang, Yuanyuan, Lin, Wei, Liu, Chang, Liu, Gang, Liu, Mengyuan, Liu, Rui, Liu, Tianyu, Liu, Wanqiang, Lu, Di'an, Lu, Peiyibin, Lu, Zhiyong, Luo, Xiyu, Ma, Sizheng, Ma, Yuanhang, Mao, Xiaoqing, Mo, Yanshan, Nie, Qiyuan, Qu, Shuiyin, Shan, Xiaolong, Shi, Gengyuan, Song, Weiming, Sun, Zhigang, Tan, Xuelin, Tang, Songsong, Tao, Mingrui, Wang, Boqin, Wang, Yue, Wang, Zhiang, Wu, Qiaoya, Wu, Xuanyi, Xia, Yuehan, Xiao, Hengyuan, Xie, Wenjin, Xu, Dacheng, Xu, Rui, Xu, Weili, Yan, Longbiao, Yan, Shengyu, Yang, Dongxin, Yang, Hang, Yang, Haoguang, Yang, Yi-Si, Yang, Yifan, Yao, Lei, Yu, Huan, Yu, Yangyi, Zhang, Aiqiang, Zhang, Bingtao, Zhang, Lixuan, Zhang, Maoxing, Zhang, Shen, Zhang, Tianliang, Zhang, Yuchong, Zhao, Qianru, Zhao, Ruining, Zheng, Shiyu, Zhou, Xiaolong, Zhu, Runyu, Zou, Yu, An, Peng, Cai, Yifu, Chen, Hongbing, Dai, Zigao, Fan, Yizhong, Feng, Changqing, Feng, Hua, Gao, He, Huang, Liang, Kang, Mingming, Li, Lixin, Li, Zhuo, Liang, Enwei, Lin, Lin, Lin, Qianqian, Liu, Congzhan, Liu, Hongbang, Liu, Xuewen, Liu, Yinong, Lu, Xiang, Mao, Shude, Shen, Rongfeng, Shu, Jing, Su, Meng, Sun, Hui, Tam, Pak-Hin, Tang, Chi-Pui, Tian, Yang, Wang, Fayin, Wang, Jianjun, Wang, Wei, Wang, Zhonghai, Wu, Jianfeng, Wu, Xuefeng, Xiong, Shaolin, Xu, Can, Yu, Jiandong, Yu, Wenfei, Yu, Yunwei, Zeng, Ming, Zeng, Zhi, Zhang, Bin-Bin, Zhang, Bing, Zhao, Zongqing, Zhou, Rong, Zhu, Zonghong
Publikováno v:
Exp. Astron. 48 (2019) 77
The Gamma-Ray Integrated Detectors (GRID) is a space mission concept dedicated to monitoring the transient gamma-ray sky in the energy range from 10 keV to 2 MeV using scintillation detectors onboard CubeSats in low Earth orbits. The primary targets
Externí odkaz:
http://arxiv.org/abs/1907.06842
Autor:
Shen, Rongfeng
Gamma-ray bursts (GRBs) are the mysterious, short and intense flashes of gamma-rays in the space, and are believed to originate from the rare, explosively devastating, stellar events that happens at cosmological distances. Enormous progress has been
Externí odkaz:
http://hdl.handle.net/2152/ETD-UT-2010-08-1880
Publikováno v:
2012, ApJ, 744, 36
The plateaus observed in about one half of the early X-ray afterglows are the most puzzling feature in gamma-ray bursts (GRBs) detected by Swift. By analyzing the temporal and spectral indices of a large X-ray plateau sample, we find that 55% can be
Externí odkaz:
http://arxiv.org/abs/1109.3453
Observational evidence suggests a link between long duration gamma ray bursts (LGRBs) and Type Ic supernovae. Here, we propose a potential mechanism for Type Ic supernovae in LGRB progenitors powered solely by accretion energy. We present spherically
Externí odkaz:
http://arxiv.org/abs/1108.1415