Multicolour modelling of SN 2013dx associated with GRB 130702A

0481173 - ASÚ 2018 RIV GB eng J - Článek v odborném periodiku
Volnova, A.A. - Pruzhinskaya, M.V. - Pozanenko, A.S. - Blinnikov, S.I. - Minaev, P.Yu. - Burkhonov, O.A. - Chernenko, A.M. - Ehgamberdiev, S.A. - Inasaridze, R.Ya. - Jelínek, Martin - Khorunzhev, G.A. - Klunko, E.V. - Krugly, Yu. N. - Mazaeva, E.D. - Rumyantsev, V.V. - Volvach, A. - Volvach, A. E.
Multicolour modelling of SN 2013dx associated with GRB 130702A.
Monthly Notices of the Royal Astronomical Society. Roč. 467, č. 3 (2017), s. 3500-3512. ISSN 0035-8711. E-ISSN 1365-2966
Institucionální podpora: RVO:67985815
Klíčová slova: gamma-ray bursts * GRB 130702A * supernovae
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.194, rok: 2017

We present optical observations of SN 2013dx, related to the Fermi burst GRB 130702A, which occurred at red shift z = 0.145. It is the second-best sampled gamma-ray burst (GRB)/supernova (SN) after SN 1998bw. The observational light curves contain more than 280 data points in the uBgrRiz filters until 88 d after the burst, and the data were collected from our observational collaboration (Maidanak Observatory, Abastumani Observatory, Crimean Astrophysical Observatory, Mondy Observatory, National Observatory of Turkey and Observatorio del Roque de los Muchachos) and from the literature. We model numerically the multicolour light curves using the one-dimensional radiation hydrodynamical code STELLA, previously widely implemented for modelling typical non-GRB SNe.
Trvalý link: http://hdl.handle.net/11104/0276777