Energy properties of long- and short-period pulsars

Details Energy properties of long- and short-period pulsars Energy properties of long- and short-period pulsars

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995azh....72..567m&link_type=abstract

Astronomicheskij Zhurnal, vol. 72, p. 567

Other

6

Pulsars, Brightness Distribution, Statistical Correlation, Magnetic Field Configurations, Luminosity, Pulse Duration

Scientific paper

The dependence of luminosity and other energy characteristics on pulsar parameters for objects with periods P equal to or greater than 1 s and P less than 1 s is analyzed. Pulsars of the first group are shown to have, on the average, lower luminosities but larger coefficients of conversion of rotational energy into radio emission. Short-period pulsars exhibit a high correlation between luminosity and magnetic-field strength near the light cylinder, as well as between luminosity and inclination of the magnetic axis to the rotation axis. These correlations are consistent with predictions of the model of emission generation in pulsars with short periods in the vicinity of the light cylinder.

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