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Constraining the Long-lived Magnetar Remnants in Short Gamma-Ray Bursts from Late-time Radio Observations

  • Authors: Liang-Duan Liu, He Gao, and Bing Zhang

2020 The Astrophysical Journal 890 102.

  • Provider: AAS Journals

Caption: Figure 1.

Comparison of the numerical results of our model with Fong et al. (2016) and Nakar & Piran (2011). The left panel is the evolution of the bulk Lorentz factor of the ejecta; the right panel is the radio lightcurves at 6 GHz. The same values for the physical parameters have been adopted to ensure a uniform comparison. The black hole model has a total kinetic energy Ek = 1050 erg.

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