A new pulsar luminosity function

Details A new pulsar luminosity function A new pulsar luminosity function

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63...78g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, Jan.-Feb. 1986, p. 78-83) Soviet Astronomy (ISSN 0038-5301), vol. 30, Jan.-Feb. 1986, p. 47-

Mathematics

2

Functions (Mathematics), Pulsars, Stellar Evolution, Stellar Luminosity, Angular Velocity, Distance, Spectral Line Width, Stellar Rotation

Scientific paper

A new pulsar luminosity function which takes the narrowing of the beam with increasing pulsar age (and decreasing spin rate) into account is calculated. The radio luminosities of the pulsars are obtained from revised distances using an intrinsic bandwidth which varies with the period following a formula proposed by Guseinov and Iusifov (1985). Numerical results are compared with those obtained using apparent pulse widths in tables and graphs.

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