OBSERVATIONS OF SUPERNOVAE ASSOCIATED WITH GAMMA-RAY BURST
A. VolnovaSpace Research Institute of the Russian Academy of Sciences, Moscow RussiaA. PozanenkoSpace Research Institute of the Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow, RussiaM. V. PruzhinskayaLomonosov Moscow State University, Sternberg Astronomical Institute, Moscow, Russia; Laboratoire de Physique Corpusculaire, Université Clermont Auvergne, Université Blaise Pascal, CNRS/IN2P3, Clermont-Ferrand, FranceС. И. БлинниковE. MazaevaSpace Research Institute of the Russian Academy of Sciences, Moscow RussiaR. Inasaridze[Abastumani Astrophysical Observatory, Ilia State University, Tbilisi, Georgia]V. T. Ayvazyan[Abastumani Astrophysical Observatory, Ilia State University, Tbilisi, Georgia]G. Inasaridze[Abastumani Astrophysical Observatory, Ilia State University, Tbilisi, Georgia]I. RevaFesenkov Astrophysical Institute, Almaty, KazakhstanО. БурхоновUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Tashkent, UzbekistanSh. A. EhgamberdievUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Tashkent, UzbekistanO. 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
ABI
Аннотация
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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