MWN Shock (Clustered Flares)

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Summary Table
Category Progenitor Type Energy Mechanism Emission Mechanism Counterparts References Brief Comments
LF Radio HF Radio Microwave Terahertz Optical/IR X-rays Gamma-rays Gravitational Waves Neutrinos
SNR (Magnetars) MWD Shock (Clustered Flares) Repeat Maser Synch. Yes Afterglow -- -- Maybe -- Low energy gamma-rays, sGRB if jet aligned Yes -- http://adsabs.harvard.edu/abs/2017ApJ...843L..26B None

Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)


Model Description

  • to use updated draft

Observational Constraints