AGN-SS: Difference between revisions
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|GWCounterpart = Yes | |GWCounterpart = Yes | ||
|NeutrinoCounterpart = Yes | |NeutrinoCounterpart = Yes | ||
|References = | |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 03:53, 11 October 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 | |||||||
| 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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