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Showing content from https://link.springer.com/article/10.1007/s00159-022-00139-w/figures/10 below:

Figure 10 | Fast radio bursts at the dawn of the 2020s

Different models of FRB emission. a Shock model from Metzger et al. (2019) where the FRB is produced at large (\(10^{10}\,\hbox {cm}\)) radii from the compact central engine (e.g., a magnetar or black hole). b Magnetospheric model from Lu et al. (2020) where the FRB is produced in the neutron star magnetosphere. Images reproduced with permission, copyright by the authors

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