Multibands fitting of Gamma-ray burst’s afterglow’s light curves using the synchrotron external forward shock model
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Springer Science and Business Media LLC
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https://link.springer.com/content/pdf/10.1007/s10509-024-04279-6.pdf
Reference88 articles.
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4. Chevalier, R.A., Li, Z.Y.: Wind interaction models for Gamma-ray burst afterglows: the case for two types of progenitors. Astrophys. J. 536(1), 195–212 (2000). https://doi.org/10.1086/308914. arXiv:astro-ph/9908272 [astro-ph]
5. Chevalier, R.A., Li, Z.Y., Fransson, C.: The diversity of Gamma-ray burst afterglows and the surroundings of massive stars. Astrophys. J. 606(1), 369–380 (2004). https://doi.org/10.1086/382867. arXiv:astro-ph/0311326 [astro-ph]
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