Xue-Feng Wu
Chinese Academy of Sciences
410 Papers
4.7K Citations
Xue-Feng Wu is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Gamma-ray burst & Afterglow. The author has an hindex of 65, co-authored 382 publications. Previous affiliations of Xue-Feng Wu include Nanjing University & California Institute of Technology.
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Papers
Fast radio bursts from the inspiral of double neutron stars
J. S. Wang,J. S. Wang,Yuan-Pei Yang,Yuan-Pei Yang,Xue-Feng Wu,Xue-Feng Wu,Zi-Gao Dai,Zi-Gao Dai,Fa-Yin Wang,Fa-Yin Wang +9 more
TL;DR: In this article, a fast radio burst (FRB) could originate from the magnetic interaction between double neutron stars (NSs) during their final inspiral within the framework of a unipolar inductor model.
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A peculiar low-luminosity short gamma-ray burst from a double neutron star merger progenitor.
Bo Zhang,Bo Zhang,Bing Zhang,Bing Zhang,Hui Sun,Wei-Hua Lei,He Gao,Ye Li,L. Shao,L. Shao,Yongheng Zhao,Y. D. Hu,Y. D. Hu,H. J. Lü,Xue-Feng Wu,Xue-Feng Wu,Xi-Long Fan,G. Wang,A. J. Castro-Tirado,A. J. Castro-Tirado,S. Zhang,B. Y. Yu,Y. Y. Cao,E. W. Liang +23 more
TL;DR: In this article, the authors show that the fluence and spectral peak energy of this event fall into the lower portion of the distribution of known short-duration gamma-ray bursts, and they also show that there are similar faint soft GRBs in the Fermi archival data, a small fraction of which might belong to this new population of nearby, low-luminosity sGRBs.
Repeating fast radio bursts from highly magnetized pulsars traveling through asteroid belts
Zi-Gao Dai,Zi-Gao Dai,J. S. Wang,J. S. Wang,Xue-Feng Wu,Xue-Feng Wu,Yong-Feng Huang,Yong-Feng Huang +7 more
TL;DR: In this paper, the authors proposed a different model, in which highly magnetized pulsars travel through the asteroid belts of other stars, and showed that a repeating fast radio burst could originate from such a pulsar encountering a large number of asteroids in the belt.
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A complete reference of the analytical synchrotron external shock models of gamma-ray bursts
TL;DR: In this paper, a review of all the analytical synchrotron external shock afterglow models by deriving the temporal and spectral indices of all models in all spectral regimes, including some regimes that have not been published before.
188
Transition from fireball to Poynting-flux-dominated outflow in the three-episode GRB 160625B
Ignacio de Gregorio Monsalvo,Ignacio de Gregorio Monsalvo,Bin-Bin Zhang,Bin-Bin Zhang,Aleksander Filip Żarnecki,Bing Zhang,Bing Zhang,A. J. Castro-Tirado,A. J. Castro-Tirado,Zi-Gao Dai,P.-H. T. Tam,X.-Y. Wang,Y. D. Hu,Y. D. Hu,Sergey Karpov,Sergey Karpov,Alexei Pozanenko,Alexei Pozanenko,Alexei Pozanenko,Fu-Wen Zhang,E. Mazaeva,P. Minaev,A. Volnova,S. R. Oates,S. R. Oats,S. R. Oats,He Gao,Xue-Feng Wu,Xue-Feng Wu,Xue-Feng Wu,Lijing Shao,Lijing Shao,Qing-Wen Tang,Gregory Beskin,Gregory Beskin,Anton Biryukov,Anton Biryukov,Sergey Bondar,E. Ivanov,E. Katkova,N. Orekhova,A. Perkov,Sasyuk,Lech Mankiewicz,Aleksander Filip Zarnecki,A. Cwiek,R. Opiela,A. K. Zadrożny,R. Aptekar,D. D. Frederiks,Dmitry S. Svinkin,A. Kusakin,R. Inasaridze,O. Burhonov,Rumyantsev,E. Klunko,A. S. Moskvitin,T. A. Fatkhullin,Sokolov,A. F. Valeev,A. F. Valeev,S. Jeong,S. Jeong,Il Han Park,M. D. Caballero-Garcia,Ronan Cunniffe,J. C. Tello,P. Ferrero,Shashi B. Pandey,Martin Jelínek,R. Sanchez-Ramirez,A. Castellon +71 more
TL;DR: In this paper, an extremely bright gamma-ray burst (GRB) 160625B was observed in both gamma and optical wavelengths, with three isolated episodes separated by long quiescent intervals, with the durations of each sub-burst being approximately 0.8, 35, and 212 seconds.
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