NS-NS Merger (Mag. Flux Change)

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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
Merger NS-NS Both Mag. flux change Curv. Yes Yes -- -- Kilonova Afterglow sGRB
if jet aligned
Yes -- http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1701.02492 In dense stellar clusters

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

Model Description

This model proposes that FRBs come from neutron star collisions in dense stellar clusters at centers of galactic nuclei.

Observational Constraints

The expectation is that FRBs would be localized to centers of galaxies, or at least would be clustered with stellar density.