Zobrazeno 1 - 10
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pro vyhledávání: '"Yuan Hao Yu"'
Autor:
Yuan, Hao-Yu, Lei, Wei-Hua
Gamma-ray bursts (GRBs), both from merger of binary compact objects (short GRBs) and collapse of massive stars (long GRBs), are expected to occur in the dense environments, e.g., the accretion disk of active galactic nuclei (AGN). The propagating of
Externí odkaz:
http://arxiv.org/abs/2408.06593
Autor:
Wang, Suo-Ning, Lü, Hou-Jun, Yuan, Yong, Yuan, Hao-Yu, Rice, Jared, Chen, Meng-Hua, Liang, En-Wei
The nearby long-duration GRB 191019A recently detected by Swift lacks an associated supernova and belongs to a host galaxy with little star formation activity, suggesting that the origin of this burst is the result of a merger of two compact objects
Externí odkaz:
http://arxiv.org/abs/2401.14418
Black hole-neutron star (BH-NS) mergers are expected to emit gravitational-wave (GW) and electromagnetic (EM) counterparts when the NS is tidally disrupted or plunges into the BH. Recently, GW 200105 and GW200115 were claimed as originating in BH-NS
Externí odkaz:
http://arxiv.org/abs/2309.13840
Autor:
Yuan, Hao-Yu, Lü, Hou-Jun, Li, Ye, Zhang, Bin-Bin, Sun, Hui, Rice, Jared, Yang, Jun, Liang, En-Wei
The growing observed evidence shows that the long- and short-duration gamma-ray bursts (GRBs) originate from massive star core-collapse and the merger of compact stars, respectively. GRB 201221D is a short-duration GRB lasting $\sim 0.1$ s without ex
Externí odkaz:
http://arxiv.org/abs/2206.07899
Autor:
Qin, Na, Deng, Jin-Ting, Liao, Jia-Jun, Liu, Xiao-Ling, Lv, Meng-Fan, Yuan, Hao-Yu, Wang, Cheng-Hua
Publikováno v:
In Food Hydrocolloids January 2025 158
Autor:
Lü, Hou-Jun, Yuan, Hao-Yu, Yi, Ting-Feng, Wang, Xiang-Gao, Hu, You-Dong, Yuan, Yong, Rice, Jared, Wang, Jian-Guo, Cao, Jia-Xin, Kong, De-Feng, Fernandez-García, Emilio, Castro-Tirado, Alberto J., Lian, Ji-Shun, Gan, Wen-Pei, Wang, Shan-Qin, Xin, Li-Ping, Caballero-García, M. D., Fan, Yu-Feng, Liang, En-Wei
Publikováno v:
ApJL, 931:L23, 2022
Long-duration gamma-ray bursts (GRBs) associated with supernovae (SNe) are believed to originate from massive star core-collapse events, whereas short-duration GRBs that are related to compact star mergers are expected to be accompanied by kilonovae.
Externí odkaz:
http://arxiv.org/abs/2201.06395
Autor:
Yang, Xing, Lü, Hou-Jun, Yuan, Hao-Yu, Rice, Jared, Zhang, Zhao, Zhang, Bin-Bin, Liang, En-Wei
Observationally, there is a small fraction of Gamma-ray bursts (GRBs) with prompt emission observed by Fermi/GBM that are composed of two pulses. Occasionally, the distance to a GRB may be lensed when a high mass astrophysical object resides in the p
Externí odkaz:
http://arxiv.org/abs/2107.11050
One possible progenitor of short gamma-ray bursts (GRBs) is thought to be from a double neutron star (NS) merger, and the remnant of such a merger may be a supramassive NS, which is supported by rigid rotation and through its survival of hundreds of
Externí odkaz:
http://arxiv.org/abs/2103.05811
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Akademický článek
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