AGN-SS: Difference between revisions

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|GWCounterpart          = Yes
|GWCounterpart          = Yes
|NeutrinoCounterpart    = Yes
|NeutrinoCounterpart    = Yes
|References            = https://arxiv.org/pdf/1709.00185.pdf
|References            = http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1709.00185
|Comments              = Neutrinos from preceding SN and from collapse to BH. GW from collapse and persistent GWs from SS.  
|Comments              = Neutrinos from preceding SN and from collapse to BH. GW from collapse and persistent GWs from SS.  
}}
}}

Revision as of 04:53, 11 October 2018





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
AGN AGN-Strange Star Interaction Repeat Electron oscillation -- Yes -- -- -- Thermal -- Yes Yes Yes http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1709.00185 Neutrinos from preceding SN and from collapse to BH. GW from collapse and persistent GWs from SS.

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


Model Description

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Observational Constraints