The unusual GRB 110709B triggered Swift/BAT twice, with a time difference of ∼11 minutes. Its light curve presented three noticeable peaks but only two were originally identified. In this work, we describe each peak as due to a different central-engine phase: the first one is the millisecond-protomagnetar stage, the second one is the BH-formation collapse phase and the last one is the Collapsar scenario with a Blandford-Znajek engine. Additionally, we analyze and explain the afterglow phase evoking the standard fireball model. Our model can successfully describe the timescales, fluxes and spectral indices observed for GRB 110709B.
CITATION STYLE
Fraija, N., Moreno-Méndez, E., & Patricelli, B. (2014). Reviewing the case of the atypical central-engine activity in GRB 110709B. In Proceedings of Science. Proceedings of Science (PoS). https://doi.org/10.22323/1.233.0093
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