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Fast X-Ray Transients Produced by Off-axis Jet Cocoons from Long Gamma-Ray Bursts

  • Authors: Jian-He Zheng, Wenbin Lu

Jian-He Zheng and Wenbin Lu 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 14.

Nonthermal X-ray “prompt emission” at Eobs = 1 keV in the observer’s frame, based on the extrapolated Band function. The jet duration is tobs = 10 s for on-axis (θv = 0°) observers. In the on-axis lightcurves, the power-law decay at tobs > 10 s arises from the high-latitude emission. The blue (θv = 0°), orange (θv = 6°), and green (θv = 8°) lightcurves correspond to different viewing angles. Solid and dashed lines are for different jet Lorentz factors of Γj = 300 and 100, respectively.

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