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GRB 170519A: Thermal Radiation in an X-Ray Flare and Decaying Magnetic Fields for the Early-time Afterglow

  • Authors: Zi-Min Zhou, Liang-Jun Chen, Rui-Quan Li, Xiang-Gao Wang, Xing-Ling, Li, En-Wei Liang, WeiKang Zheng, Alexei V. Filippenko

Zi-Min Zhou et al 2025 The Astrophysical Journal 984 .

  • Provider: AAS Journals

Caption: Figure 8.

Relations between photospheric parameters during Pulse III (Flare II), where the slices with ΔBIC > 2 are included. Top panel: the LBB–ΓBB plane for Pulse III (Flare II), where the dashed line represents the relation ﹩{{\rm{\Gamma }}}_{{\rm{BB}}}\propto {L}_{{\rm{BB}}}^{0.27}﹩. Bottom panel: relation between kT and LBB, where the solid line represents the fitting result LBB ∼ kT2.54±0.17 and the dashed line represents LBB ∼ kT4.

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