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Statistical study of high energy radiation from rotation-powered pulsars

descriptionPublicationkeyboard_double_arrow_right Article 06 Sep 2010 China (People's Republic of) English Publisher:Science in China Press. The Journal's web site is located at http://www.scichina.com:8081/sciAe/EN/volumn/current.shtml
Authors: Cheng, KS; Zhang, L;

handle: 10722/80389

Statistical study of high energy radiation from rotation-powered pulsars

Abstract

Based on our self-consistent outer gap model for high energy emission from the rotationpowered pulsars, we study the statistical properties of X-ray and γ-ray emission from the rotation-powered pulsars, and other statistical properties (e. g. diffuse γ-ray background and unidentified γ-ray point sources) related to γ-ray pulsars in our Galaxy and nearby galaxies are also considered.

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Country
China (People's Republic of)
Related Organizations
Keywords

Statistics, Gamma rays, General-stars, Theory-pulsars, Neutron-stars

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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