Pulse-interpulse interaction in pulsar PSR 1822-09

Details Pulse-interpulse interaction in pulsar PSR 1822-09 Pulse-interpulse interaction in pulsar PSR 1822-09

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...109..279f&link_type=abstract

Astronomy and Astrophysics, vol. 109, no. 2, May 1982, p. 279-281. Research supported by the Alexander von Humboldt-Stiftung an

Astronomy and Astrophysics

Astrophysics

28

Emission Spectra, Periodic Variations, Pulsars, Radio Spectra, Stellar Magnetic Fields, Propagation Modes, Pulsar Magnetospheres, Radio Emission, Stellar Models

Scientific paper

In an analysis of single-pulse data from both the main pulse and the interpulse of PSR 1822-09, the subpulse properties are exploited to test ideas concerning the site of the radio emission in the pulsar magnetosphere. Main pulse and interpulse profiles for selected subpulses at the leading and trailing edges of the main pulse window are shown, together with the main pulse and interpulse profiles for the Q and B modes. It is found that the inter-pulse appears to participate in the mode-change, but not in a manner which conforms simply with any current model for pulsar emission.

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