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Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets. I. A Systematic Study

  • Authors: Haocheng Zhang, Xiaocan Li, Dimitrios Giannios, Fan Guo, Yi-Hsin Liu, and Lingyi Dong

2020 The Astrophysical Journal 901 149.

  • Provider: AAS Journals

Caption: Figure 12.

From top to bottom: optical light curves, temporal PD, and PA for different magnetization factors (they are MF1, default run, and MF2). Notice that we rescale the light curves of runs MF1 and MF2 by factors of 5 and 0.5, respectively, to make them appear on the same scale as the default run.

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