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The Radio Interpulse from PSR 0950+08

Published online by Cambridge University Press:  14 August 2015

T. H. Hankins  and
J. M. Cordes
T. H. Hankins
Affiliation:
National Astronomy and Ionosphere Center
J. M. Cordes
Affiliation:
National Astronomy and Ionosphere Center

Extract

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Two hypotheses exist to explain the radio interpulse of PSR 0950+08 within the context of polar cap emission models:

  1. 1) The emission originates at a single magnetic pole as for other two-component pulsars, except that the component spacing is much wider.

  2. 2) The interpulse emission originates at the opposite magnetic pole. We discuss here some new observations and their implications for the single and double pole hypotheses.

Type
III. Radio Observations of Pulsars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 207 - 209
Copyright
Copyright © Reidel 1981 

References

Cordes, J.M.: 1978, Astrophys. J. 222, p. 1006.CrossRefGoogle Scholar
Hankins, T.H. and Boriakoff, V.: 1978, Nature 276, p. 45.CrossRefGoogle Scholar
Hankins, T.H. and Boriakoff, V.: 1980, Nature, in press.Google Scholar
Manchester, R.N.: 1978, Proc. Astron. Soc. Australia 3, p. 200.CrossRefGoogle Scholar