Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249..241h&link_type=abstract
Astrophysical Journal, Part 1, vol. 249, Oct. 1, 1981, p. 241-253. Research supported by the National Astronomy and Ionosphere
Astronomy and Astrophysics
Astronomy
56
Pulsars, Pulse Duration, Pulsed Radiation, Stellar Radiation, Fluctuation Theory, Frequency Response, Stellar Models, Stellar Rotation
Scientific paper
Consideration of the frequency dependence of emission over the entire pulse period shows that: (1) interpulse emission is accompanied by low level emission over at least 83% of the rotation period; (2) individual interpulses may be as strong as 60% of the average main pulse, by comparison to an average interpulse-main pulse ratio of 2%; (3) interpulses are correlated with main pulses; and (4) the interpulse-main pulse separation is frequency-independent between 100 and 5000 MHz, while (5) the average interpulse and main pulse widths vary as the -0.5 + or - 0.05 power of nu below 400 MHz. In addition, single-pole and double-pole models are considered and found to require additional ad hoc additions to explain the observations. The simplest alternative is the modification of the single-pole models in which the magnetic axis is nearly aligned with the rotation axis.
Cordes James M.
Hankins Timothy H.
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