Unusual frequency dependence of the linear polarization of the radio emission of the pulsar B0329 + 54

Details Unusual frequency dependence of the linear polarization of the radio emission of the pulsar B0329 + 54 Unusual frequency dependence of the linear polarization of the radio emission of the pulsar B0329 + 54

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..252s&link_type=abstract

Astronomy Reports, Volume 42, Issue 2, March 1998, pp.252-258

Astronomy and Astrophysics

Astronomy

5

Scientific paper

The degree of linear polarization of the radio emission of the pulsar B0329+54 at 60 and 103 MHz is more than twice that expected based on its frequency dependence at higher frequencies. Variation of the spectral behavior is observed in the frequency range 100-300 MHz for at least three parameters of the pulsar emission: the distance between the central and trailing components in the intensity profile, the width of the central component, and the degree of linear polarization. The two outer components in the integrated profile have qualitatively different spectral behavior with regard to their distance from the central component.

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