Image Details

Choose export citation format:

Internal Shock with a Background Magnetic Field for the Prompt Emission of Gamma-Ray Bursts—A Case Study of GRB 211211A

  • Authors: Li Zhou, Da-Bin Lin, Xing Yang, Guo-Yu Li, Kuan Liu, Jing Li, En-Wei Liang

Li Zhou et al 2023 The Astrophysical Journal 957 .

  • Provider: AAS Journals

Caption: Figure 2.

Radiation spectra of our model with different parameters, where the fiducial case (green solid line) in each panel is the same as that in Figure 1. (a) Different values of α B are indicated by different dashed lines, i.e., α B = 0 (black), 0.5 (red), 2 (blue), and 4 (wine). (b) Different values of p are indicated by different dashed lines, i.e., p = 2.5 (black), 3 (red), and 4 (blue). (c) Different values of R dis are indicated by different dashed lines, i.e., R dis = 1014 (black), 3 × 1014 (blue), 3 × 1015 (red), and 1016 cm (gray). (d) Different values of ﹩\gamma {{\prime} }_{{\rm{m}}}={10}^{4}﹩ (blue dashed line), or Y 0 = 2 (red dashed line), or ﹩t{{\prime} }_{\mathrm{end}}=3﹩ (orange dashed line), or τ B = 0.001 (magenta dashed line) are adopted.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse