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

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00580631" target="_blank" >RIV/67985815:_____/23:00580631 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/23:00580631 RIV/68407700:21230/23:00367123

  • Result on the web

    <a href="https://doi.org/10.1038/s41550-023-01972-4" target="_blank" >https://doi.org/10.1038/s41550-023-01972-4</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1038/s41550-023-01972-4" target="_blank" >10.1038/s41550-023-01972-4</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

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

  • Original language description

    Long gamma-ray bursts are produced by energy dissipation within ultra-relativistic jets launched by newborn black holes after the collapse of a peculiar class of massive stars. Right after the luminous and highly variable gamma-ray emission, a multi-wavelength afterglow is released by external dissipation of the jet energy in the medium that surrounds the progenitor star. We report the discovery of a very bright (~10 mag) optical emission ~28 s after the explosion of the extremely luminous and energetic GRB 210619B located at redshift 1.937. We observed the transition from a bright reverse to the forward shock emission, demonstrating that the early and late gamma-ray-burst multi-wavelength emission originated from a narrow, magnetized jet propagating into a rarefied interstellar medium. These conditions are found to be optimal to produce the bright optical flash from the reverse shock.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Nature Astronomy

  • ISSN

    2397-3366

  • e-ISSN

    2397-3366

  • Volume of the periodical

    7

  • Issue of the periodical within the volume

    7

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    11

  • Pages from-to

    843-855

  • UT code for WoS article

    000986017100002

  • EID of the result in the Scopus database

    2-s2.0-85159370215