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. Author manuscript; available in PMC: 2021 Oct 12.
Published in final edited form as: Astrophys J. 2019 Jul 10;879(2):91. doi: 10.3847/1538-4357/ab258e

Figure 7.

Figure 7.

Synchrotron intensity averaged over a region around the current location of Geminga with a radius of 1° for scenarios A through D. Also shown are the results for a model where Geminga is stationary with (rz, rt) = (30, 50) pc and γ1 2.0.