Radio rebrightening of the GRB afterglow by the accompanying supernova

@article{Duran2015RadioRO,
  title={Radio rebrightening of the GRB afterglow by the accompanying supernova},
  author={Rodolfo Barniol Duran and Dimitrios Giannios},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2015},
  volume={454},
  pages={1711-1718}
}
  • R. Duran, D. Giannios
  • Published 23 April 2015
  • Physics
  • Monthly Notices of the Royal Astronomical Society
The gamma-ray burst (GRB) jet powers the afterglow emission by shocking the surrounding medium, and radio afterglow can now be routinely observed to almost a year after the explosion. Long-duration GRBs are accompanied by supernovae (SNe) that typically contain much more energy than the GRB jet. Here we consider the fact that the SN blast wave will also produce its own afterglow, which will peak at much later time (since it is non-relativistic), when the SN blast wave transitions from a… 

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