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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 3.

The angular distributions of the isotropic-equivalent energy Eiso (solid lines, left axis) and the photospheric four-velocity uph (dashed lines, right axis) for the four models. The blue, red, green, and purple lines correspond to models Lc, Lw, LI, and Llow, respectively. The upper panel shows the distribution at ﹩{R}_{{\rm{c}},{\rm{\max }}}\approx 1{0}^{12}\,{\rm{cm}}﹩, while the lower panel shows shows those at ﹩{R}_{{\rm{c}},{\rm{\max }}}\approx 1{0}^{13}\,{\rm{cm}}﹩.

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