Variable Stars: Difference between revisions
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== Observational Constraints == | == Observational Constraints == | ||
Multiple peaks are possible. For this model to hold, one must observe a positive frequency sweep ahead of a negative frequency sweep. | |||
Revision as of 08:46, 2 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 | |||||||
| Other | Variable Stars | Repeat | Undulator | Synch. | Yes | -- | -- | -- | -- | -- | -- | -- | -- | http://adsabs.harvard.edu/abs/2018MNRAS.477.2470L | None |
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
Multiple peaks are possible. For this model to hold, one must observe a positive frequency sweep ahead of a negative frequency sweep.