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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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. |
doi_str_mv | 10.48550/arxiv.2109.00010 |
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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. 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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.</description><subject>Black holes</subject><subject>Ejecta</subject><subject>Emission</subject><subject>Gamma ray bursts</subject><subject>Gamma rays</subject><subject>Interstellar matter</subject><subject>Massive stars</subject><subject>Red shift</subject><subject>Shock wave propagation</subject><subject>Shock waves</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNjcFqwkAURYeCYKj5gO4edGMXiTOTTIzrYnEtLgPhNY46kmT0vYnYv-8s-gFdXTj3XK4Qb0rmZW2MXCE93SPXSm5yKaWSLyLRRaGyutR6LlLma8S6WmtjikTst8_O3oLzI_b9D3yTO18C-Eg67MEOjjl2cCI_AAIhWcDxCEfHAccAzbI54zBg1nwQxvlEHBZidsKebfqXr-L9a3v43GU38vfJcmivfqL4x602VV1KpdS6-J_1CzPHRas</recordid><startdate>20211121</startdate><enddate>20211121</enddate><creator>Gor Oganesyan</creator><creator>Karpov, Sergey</creator><creator>Jelínek, Martin</creator><creator>Beskin, Gregory</creator><creator>Ronchini, Samuele</creator><creator>Banerjee, Biswajit</creator><creator>Branchesi, Marica</creator><creator>Štrobl, Jan</creator><creator>Polášek, Cyril</creator><creator>Hudec, René</creator><creator>Ivanov, Eugeny</creator><creator>Katkova, Elena</creator><creator>Perkov, Alexey</creator><creator>Biryukov, Anton</creator><creator>Lyapshina, Nadezhda</creator><creator>Sasyuk, Vyacheslav</creator><creator>Mašek, Martin</creator><creator>Janeček, Petr</creator><creator>Ebr, Jan</creator><creator>Juryšek, Jakub</creator><creator>Cunniffe, Ronan</creator><creator>Prouza, Michael</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20211121</creationdate><title>Exceptionally bright optical emission from a rare and distant \(\gamma-\)ray burst</title><author>Gor Oganesyan ; 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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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