Stellar Coronae: Difference between revisions

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|GWCounterpart          = N/A
|GWCounterpart          = N/A
|NeutrinoCounterpart    = N/A
|NeutrinoCounterpart    = N/A
|References            = https://arxiv.org/pdf/1009.5392.pdf, http://adsabs.harvard.edu/abs/2014ApJ...797...70K
|References            = https://arxiv.org/pdf/1310.2419.pdf, http://adsabs.harvard.edu/abs/2015MNRAS.454.2183M
|Comments              = None
|Comments              = None
}}
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Revision as of 07:09, 2 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
Void Stellar Corona N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A https://arxiv.org/pdf/1310.2419.pdf, http://adsabs.harvard.edu/abs/2015MNRAS.454.2183M None

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


Model Description

    • To fill in with updated draft

Observational Constraints

N/A