Simultaneous radio and optical polarimetry of GRB 191221B afterglow

0583711 - ASÚ 2024 RIV US eng J - Článek v odborném periodiku
Urata, Y. … celkem 19 autorů
Simultaneous radio and optical polarimetry of GRB 191221B afterglow.
Nature Astronomy. Roč. 7, January (2023), s. 80-87. ISSN 2397-3366. E-ISSN 2397-3366
Výzkumná infrastruktura: EU-ARC.CZ III - 90259
Klíčová slova: gamma-ray bursts * relativistic collisionless * shocks light curves
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 14.1, rok: 2022
Způsob publikování: Omezený přístup
https://doi.org/10.1038/s41550-022-01832-7

Gamma-ray bursts (GRBs) are the most luminous transients in the universe and are utilized as probes of early stars, gravitational wave counterparts and collisionless shock physics. In spite of studies on polarimetry of GRBs in individual wavelengths that characterized intriguing properties of prompt emission and afterglow, no coordinated multi-wavelength measurements have yet been performed. Here we report the first coordinated simultaneous polarimetry in the optical and radio bands for the afterglow associated with the typical long GRB 191221B. Our observations successfully caught the radio emission, which is not affected by synchrotron self-absorption, and show that the emission is depolarized in the radio band compared with the optical one. Our simultaneous polarization angle measurement and temporal polarization monitoring indicate the existence of cool electrons that increase the estimate of jet kinetic energy by a factor of more than 4 for this GRB afterglow. Further coordinated multi-wavelength polarimetric campaigns would improve our understanding of the total jet energies and magnetic field configurations in the emission regions of various types of GRBs, which are required to comprehend the mass scales of their progenitor systems and the physics of collisionless shocks.
Trvalý link: https://hdl.handle.net/11104/0351706