O
O. Burhonov
Publications - 4
Citations - 213
O. Burhonov is an academic researcher. The author has contributed to research in topics: Gamma-ray burst & Luminosity. The author has an hindex of 2, co-authored 3 publications receiving 160 citations.
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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.
Posted Content
Transition from Fireball to Poynting-flux-dominated Outflow in Three-Episode GRB 160625B
Bin-Bin Zhang,Bing Zhang,A. J. Castro-Tirado,Zi-Gao Dai,P.-H. T. Tam,X.-Y. Wang,Y. D. Hu,Sergey Karpov,A. Pozanenko,Fu-Wen Zhang,E. Mazaeva,P. Minaev,A. Volnova,S. R. Oates,He Gao,Xue-Feng Wu,Lijing Shao,Qing-Wen Tang,Gregory Beskin,Anton Biryukov,Sergey Bondar,E. Ivanov,E. Katkova,N. Orekhova,A. Perkov,V. Sasyuk,Lech Mankiewicz,A. F. Zarnecki,A. Cwiek,R. Opiela,A. Zadrozny,R. Aptekar,D. D. Frederiks,Dmitry S. Svinkin,A. V. Kusakin,R. Inasaridze,O. Burhonov,Vasilij Rumyantsev,E. Klunko,A. S. Moskvitin,T. A. Fatkhullin,V. V. Sokolov,A. F. Valeev,S. Jeong,Il Han Park,M. D. Caballero-Garcia,R. Cunniffe,J. C. Tello,P. Ferrero,S. B. Pandey,Martin Jelínek,F. K. Peng,R. Sanchez-Ramirez,A. Castellon +53 more
TL;DR: In this paper, the authors reported an extraordinarily bright gamma-ray burst (GRB) 160625B, simultaneously observed in gamma-rays and optical wavelengths, whose prompt emission consists of three isolated episodes separated by long quiescent intervals, with the durations of each "sub-burst" being $ 0.8 s, 35 s, and 212 s, respectively.
Journal ArticleDOI
Publisher Correction: Transition from fireball to Poynting-flux-dominated outflow in the three-episode GRB 160625B
Bin-Bin Zhang,Bin-Bin Zhang,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,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,V. Sasyuk,Lech Mankiewicz,Aleksander Filip Żarnecki,A. Cwiek,R. Opiela,A. K. Zadrożny,R. Aptekar,D. D. Frederiks,Dmitry S. Svinkin,A. Kusakin,R. Inasaridze,O. Burhonov,Vasilij Rumyantsev,E. Klunko,A. S. Moskvitin,T. A. Fatkhullin,V. V. 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,F. K. Peng,R. Sanchez-Ramirez,A. Castellon +67 more
TL;DR: In the version of this letter originally published, the letter i was mistakenly omitted from the surname of the author R. Sanchez-Ramirez as discussed by the authors. This has now been corrected.
Journal ArticleDOI
The Early Light Curve of the Type Ia Supernova 2021hpr in NGC 3147: Progenitor Constraints with the Companion Interaction Model
G. Lim,Myungshin Im,Gregory S. H. Paek,Sung-Chul Yoon,Changsu Choi,Sophia Kim,J. Craig Wheeler,Benjamin P. Thomas,J'ozsef Vink'o,Dohyeong Kim,Jinguk Seo,Won-Seok Kang,Taewoo Kim,H.-I. Sung,Yonggi Kim,Joh-Na Yoon,Hae-Yeon Kim,Jeong-Gyu Kim,Hana Bae,Sh. A. Ehgamberdiev,O. Burhonov,D. O. Mirzaqulov +21 more
TL;DR: In this article , the early part of the BVRI-band light curves were fitted with a two-component model consisting of ejecta-companion interaction and a simple power-law model, and the early excess light in the multiband light curve supported a nondegenerate companion in the progenitor system of SN 2021hpr.