PSR 0950 + 08 - A model for interpulse emission

Details PSR 0950 + 08 - A model for interpulse emission PSR 0950 + 08 - A model for interpulse emission

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..267g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 2, Nov. 1983, p. 267-270.

Astronomy and Astrophysics

Astrophysics

25

Pulsars, Stellar Models, Astronomical Models, Frequency Response, Lines Of Force, Magnetic Poles, Stellar Radiation

Scientific paper

Following Hankins and Cordes (1981), the single-pole model for pulsar is further developed, assuming the magnetic axis to be nearly aligned to the rotation axis. The model accounts for the observed fact that the main pulse to interpulse separation is less than 180°, and independent to frequency. It also explains why interpulses tend to occur in short period pulsars and at low frequencies.

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