Model pulsar radio spectra and pulse profiles

Details Model pulsar radio spectra and pulse profiles Model pulsar radio spectra and pulse profiles

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63...62k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, Jan.-Feb. 1986, p. 62-70) Soviet Astronomy (ISSN 0038-5301), vol. 30, Jan.-Feb. 1986, p. 38-

Astronomy and Astrophysics

Astronomy

7

Emission Spectra, Pulsars, Radio Spectra, Spectral Energy Distribution, Stellar Models, Stellar Spectrophotometry

Scientific paper

A quantitative analysis of pulsars' radio emission in the framework of the hollow-cone and curvature-radiation model was made. The authors indicate a possibility of fitting this model to the observed spectra, including decreasing steepness at lower frequencies followed by low-frequency cutoff, and to the observed integrated profiles including their frequency evolution. They have determined the frequency dependence of the radius of the emitting region, the energy spectrum of emitting particles and its radial distribution which provided such fitting. They propose to use the scheme considered for mathematical modeling of the characteristics of pulsar radio emission.

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