A
A. S. Moskvitin
Researcher at Russian Academy of Sciences
Publications - 33
Citations - 683
A. S. Moskvitin is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Gamma-ray burst & Supernova. The author has an hindex of 10, co-authored 33 publications receiving 557 citations. Previous affiliations of A. S. Moskvitin include Kazan Federal University.
Papers
More filters
Journal ArticleDOI
The unusual γ-ray burst GRB 101225A from a helium star/neutron star merger at redshift 0.33
Christina C. Thöne,Christina C. Thöne,A. de Ugarte Postigo,Chris L. Fryer,K. L. Page,Javier Gorosabel,Miguel A. Aloy,Daniel A. Perley,Chryssa Kouveliotou,Hans-Thomas Janka,Petar Mimica,Judith Racusin,H. A. Krimm,H. A. Krimm,Jay Cummings,S. R. Oates,Stephen T. Holland,Stephen T. Holland,M. H. Siegel,M. de Pasquale,Eda Sonbas,Eda Sonbas,Myungshin Im,Wonsun Park,D. A. Kann,Sergei Guziy,L. Hernández García,A. Llorente,K. Bundy,C. Choi,H. Jeong,Heidi Korhonen,Heidi Korhonen,Petr Kubánek,Junghyun Lim,A. S. Moskvitin,T. Muñoz-Darias,Soojong Pak,I. Parrish +38 more
TL;DR: The proposed progenitor is a merger of a helium star with a neutron star that underwent a common envelope phase, expelling its hydrogen envelope, creating a GRB-like jet which became thermalized by interacting with the dense, previously ejected material, thus creating the observed black body, until finally the emission from the supernova dominated.
Journal ArticleDOI
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.
Journal ArticleDOI
GRB 170817A Associated with GW170817: Multi-frequency Observations and Modeling of Prompt Gamma-Ray Emission
Alexei Pozanenko,Alexei Pozanenko,Maxim V. Barkov,P. Yu. Minaev,A. Volnova,E. Mazaeva,A. S. Moskvitin,M. A. Krugov,V. A. Samodurov,V. M. Loznikov,Maxim Lyutikov +10 more
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
Photometry and spectroscopy of the luminous red nova PSNJ14021678+5426205 in the galaxy M101
V. P. Goranskij,E. A. Barsukova,O. I. Spiridonova,A. F. Valeev,A. F. Valeev,T. A. Fatkhullin,A. S. Moskvitin,O. V. Vozyakova,D. V. Cheryasov,Boris Safonov,A. V. Zharova,T. Hancock +11 more
TL;DR: In this paper, the authors present the results of the study of a red nova from the observations carried out with the Russian 6m telescope (BTA) along with other telescopes of SAO RAS and SAI MSU.