MWN Shock (Clustered Flares): Difference between revisions
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Emma Platts (talk | contribs) (Created page with " <!-- Brings in the summary table --> <!-- This is an example. Change the right hand side of all these assignments --> {{FRBTableTemplate |Category = SNR (Magne...") |
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Revision as of 09:01, 27 September 2018
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