NS Combing: Difference between revisions

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|GWCounterpart          = --
|GWCounterpart          = --
|NeutrinoCounterpart    = --
|NeutrinoCounterpart    = --
|References            = http://adsabs.harvard.edu/abs/2017ApJ...836L..32Z, https://arxiv.org/pdf/1801.05436.pdf
|References            = http://adsabs.harvard.edu/abs/2017ApJ...836L..32Z, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1801.05436
|Comments              = The model can apply to a variety of events, and thus counterparts will depend on the scenario.
|Comments              = The model can apply to a variety of events, and thus counterparts will depend on the scenario.
}}
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Revision as of 05:42, 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
Other NS Combing Both Various Mag. reconnection Yes -- -- -- -- -- -- -- -- http://adsabs.harvard.edu/abs/2017ApJ...836L..32Z, http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1801.05436 The model can apply to a variety of events, and thus counterparts will depend on the scenario.

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


Model Description

To be filled in with updated draft

Observational Constraints

To be filled in with updated draft