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GRB 190919B: Rapid optical rise explained as a flaring activity

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JELÍNEK Martin TOPINKA Martin KARPOV Sergey MALEŇÁKOVÁ Alžběta HU Y.-D. RIGOSELLI Michela ŠTROBL Jan EBR Jan CUNNIFFE Ronan THOENE Christina MAŠEK Martin JANEČEK Petr FERNANDEZ-GARCÍA Emilio HIRIART David LEE William H. VÍTEK Stanislav HUDEC René TRÁVNÍČEK Petr CASTRO-TIRADO Alberto J. PROUZA Michael

Rok publikování 2022
Druh Článek v odborném periodiku
Časopis / Zdroj Astronomy and Astrophysics
Fakulta / Pracoviště MU

Přírodovědecká fakulta

Citace
www https://www.aanda.org/articles/aa/full_html/2022/06/aa43010-21/aa43010-21.html
Doi http://dx.doi.org/10.1051/0004-6361/202143010
Klíčová slova techniques; photometric; gamma-ray burst; individual; GRB190919B
Popis Following the detection of a long GRB 190919B by INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory), we obtained an optical photometric sequence of its optical counterpart. The light curve of the optical emission exhibits an unusually steep rise similar to 100 s after the initial trigger. This behaviour is not expected from a 'canonical' GRB optical afterglow. As an explanation, we propose a scenario consisting of two superimposed flares: an optical flare originating from the inner engine activity followed by the hydrodynamic peak of an external shock. The inner-engine nature of the first pulse is supported by a marginal detection of flux in hard X-rays. The second pulse eventually concludes in a slow constant decay, which, as we show, follows the closure relations for a slow cooling plasma expanding into the constant interstellar medium and can be seen as an optical afterglow sensu stricto.

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