Exceptionally bright optical emission from a rare and distant \(\gamma-\)ray burst

Long \(\rm \gamma\)-ray bursts (GRBs) are produced by the dissipation of ultra-relativistic jets launched by newly-born black holes after the collapse of massive stars. Right after the luminous and highly variable \(\gamma\)-ray emission, the multi-wavelength afterglow is released by the external di...

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Hauptverfasser: Gor Oganesyan, Karpov, Sergey, Jelínek, Martin, Beskin, Gregory, Ronchini, Samuele, Banerjee, Biswajit, Branchesi, Marica, Štrobl, Jan, Polášek, Cyril, Hudec, René, Ivanov, Eugeny, Katkova, Elena, Perkov, Alexey, Biryukov, Anton, Lyapshina, Nadezhda, Sasyuk, Vyacheslav, Mašek, Martin, Janeček, Petr, Ebr, Jan, Juryšek, Jakub, Cunniffe, Ronan, Prouza, Michael
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container_title arXiv.org
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creator Gor Oganesyan
Karpov, Sergey
Jelínek, Martin
Beskin, Gregory
Ronchini, Samuele
Banerjee, Biswajit
Branchesi, Marica
Štrobl, Jan
Polášek, Cyril
Hudec, René
Ivanov, Eugeny
Katkova, Elena
Perkov, Alexey
Biryukov, Anton
Lyapshina, Nadezhda
Sasyuk, Vyacheslav
Mašek, Martin
Janeček, Petr
Ebr, Jan
Juryšek, Jakub
Cunniffe, Ronan
Prouza, Michael
description Long \(\rm \gamma\)-ray bursts (GRBs) are produced by the dissipation of ultra-relativistic jets launched by newly-born black holes after the collapse of massive stars. Right after the luminous and highly variable \(\gamma\)-ray emission, the multi-wavelength afterglow is released by the external dissipation of the jet in circumburst medium. We report the discovery of a very bright (\(\rm \sim 10\) mag) optical emission \(\rm \sim 28\) s after the explosion of the extremely luminous and energetic GRB 210619B located at redshift 1.937. Early multi-filter observations allowed us to witness the end of the shock wave propagation into the GRB ejecta. We observed the spectral transition from a bright reverse to the forward shock emission, demonstrating that the early and late GRB multi-wavelength emission is originated from a very narrow jet propagating into an unusually rarefied interstellar medium. We also find evidence of an additional component of radiation, coming from the jet wings which is able explain the uncorrelated optical/X-ray emission.
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subjects Black holes
Ejecta
Emission
Gamma ray bursts
Gamma rays
Interstellar matter
Massive stars
Red shift
Shock wave propagation
Shock waves
title Exceptionally bright optical emission from a rare and distant \(\gamma-\)ray burst
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