NS and Asteroid Belt - Revision history

Emma Platts at 16:43, 16 October 2018

2018-10-16T16:43:35Z

← Older revision		Revision as of 12:43, 16 October 2018
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	\|GWCounterpart = --		\|GWCounterpart = --
	\|NeutrinoCounterpart = --		\|NeutrinoCounterpart = --
	\|References = http://adsabs.harvard.edu/abs/2016ApJ...829...27D		\|References = http://adsabs.harvard.edu/abs/2016ApJ...829...27D, http://iopscience.iop.org/article/10.3847/2041-8213/aa65c9/pdf
	\|Comments = None		\|Comments = None
	}}		}}

Apw at 11:22, 10 October 2018

2018-10-10T11:22:07Z

← Older revision		Revision as of 07:22, 10 October 2018
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	== Model Description ==		== Model Description ==

	* to ~~add~~		Consider an asteroid belt surrounding a star. If a pulsar passes through this system, it is likely to encounter multiple asteroids. When this happens, charged particles may be stripped from the asteroidal surface into the NS magnetosphere, where they are accelerated to ultra-relativistic speeds, resulting in coherent curvature radiation.

	== Observational Constraints ==		== Observational Constraints ==

			The time between edge on collisions within the asteroid belt is consistent with the time between the signals of FRB 121102.

Emma Platts at 13:12, 2 October 2018

2018-10-02T13:12:33Z

← Older revision		Revision as of 09:12, 2 October 2018
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	\|Category = Collision/ Interaction		\|Category = Collision/ Interaction
	\|Progenitor = NS and Asteroid Belt		\|Progenitor = NS and Asteroid Belt
	\|Type = ~~Repeating~~		\|Type = Repeat
	\|EnergyMechanism = Electron stripping		\|EnergyMechanism = Electron stripping
	\|EmissionMechanism = Curv.		\|EmissionMechanism = Curv.

Emma Platts: Created page with " {{FRBTableTemplate |Category = Collision/..."

2018-09-27T14:44:33Z

Created page with "   {{FRBTableTemplate |Category = Collision/..."

New page

{{FRBTableTemplate
|Category = Collision/ Interaction
|Progenitor = NS and Asteroid Belt
|Type = Repeating
|EnergyMechanism = Electron stripping
|EmissionMechanism = Curv.
|LFRadioCounterpart = Yes
|HFRadioCounterpart = --
|MicrowaveCounterpart = --
|THzCounterpart = --
|OIRCounterpart = --
|XrayCounterpart = --
|GammarayCounterpart = Yes
|GWCounterpart = --
|NeutrinoCounterpart = --
|References = http://adsabs.harvard.edu/abs/2016ApJ...829...27D
|Comments = None
}}

== Model Description ==

* to add

== Observational Constraints ==