OBSERVATIONS OF SUPERNOVAE ASSOCIATED WITH GAMMA-RAY BURST
A. VolnovaSpace Research Institute of the Russian Academy of Sciences, Moscow RussiaA. PozanenkoSpace Research InstituteM. V. PruzhinskayaUniversity of Clermont AuvergneС. И. БлинниковE. MazaevaSpace Research Institute of the Russian Academy of Sciences, Moscow RussiaR. InasaridzeEvgeni Kharadze Georgian National Astrophysical ObservatoryV. T. Ayvazyan[Abastumani Astrophysical Observatory, Ilia State University, Tbilisi, Georgia]G. InasaridzeEvgeni Kharadze Georgian National Astrophysical ObservatoryI. RevaFesenkov Astrophysical Institute, Almaty, KazakhstanО. БурхоновUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Tashkent, UzbekistanSh. A. EhgamberdievUlugh Beg Astronomical InstituteO. Kvaratskhelia[Abastumani Astrophysical Observatory, Ilia State University, Tbilisi, Georgia]V. RumyantsevCrimean Astrophysical Observatory, Nauchniy, Crimea, RussiaYuri KruglyE. KlunkoInstitute of Solar-Terrestrial Physics, Russian Academy of Sciences, Siberian branch, Irkutsk, RussiaI. Molotov‡Keldysh Institute of Applied Mathematics, Moscow, Russia
2018en
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Annotatsiya
In this paper, we present an overview of the observational properties of supernovae (SNe) associated with long-duration gamma- ray bursts (GRBs). We summarise the statistics of GRB-SNe physical properties and consider different modelling methods. We report the results of the numerical modelling of the GRB 130702A/SN 2013dx multicolour light curve using a spherically symmetrical multi-group radiation hydrodynamics code STELLA. We have obtained main bolometric parameters of the SN and compare our results with those of analytical modelling.
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