The pulse profile of γ-ray pulsars and the emission region geometry

Details The pulse profile of γ-ray pulsars and the emission region geometry The pulse profile of γ-ray pulsars and the emission region geometry

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..643m&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 643-647 (1997).

Computer Science

Pulsars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

γ-ray pulsars are grouped in two classes: ``double-peaked'' (D) and ``single-peaked'' (S) pulsars. D pulsars have phase separation between the peaks in the range 0.4-0.5, while S pulsars show broad peaks. We evaluated for two geometrical models of the emission region (polar cone and outer gap models) the probabilities to detect a D or a S pulsar, and the corresponding distribution of the peak separation and conclude that both these models are not able to explain the lack of D sources with separation less than 0.4.

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