Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/ The Astrophysical Jo...arrow_drop_down
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
The Astrophysical Journal
Article . 1989 . Peer-reviewed
Data sources: Crossref
https://dx.doi.org/10.1086/167...
Article
Data sources: Microsoft Academic Graph
 View all 1 versions
Claim

Spectra of Crab-like pulsars

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1989 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 342, page 396 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Cheng Ho;

doi: 10.1086/167600

Spectra of Crab-like pulsars

Abstract

Un modele est construit pour le rayonnement energetique resultant de la formation d'une region de depletion des charges (gap) dans la magnetosphere exterieure des pulsars en rotation rapide. Le modele utilise une procedure iterative avec un parametre variant qui represente la fraction lineaire de la magnetosphere occupee par le gap. Les spectres sont calcules pour le pulsar du Crabe et le pulsar 50 ms PSR 0540-693 dans le Grand Nuage de Magellan. Le spectre d'un pulsar 15 ms hypothetique restant apres l'episode de SN 1987A est presente et la detectabilite de la pulsation est discutee

  • BIP!
    Impact byBIP!
    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).
    		 32
    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.
    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Top 10%
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    		 Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
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!
32
Average
Top 10%
Average
gold