Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...101..356w&link_type=abstract
Astronomy and Astrophysics, vol. 101, no. 3, Sept. 1981, p. 356-361. Research supported by Alexander von Humboldt-Stiftung.
Astronomy and Astrophysics
Astrophysics
28
Astronomical Models, Drift Rate, Propagation Modes, Pulsars, Pulsed Radiation, Stellar Radiation, Polar Caps, Power Spectra, Spectrum Analysis, Stellar Spectra
Scientific paper
We report observations of the long-period pulsar PSR 2319+60 at t4t5 MHz. When not in a null state, the pulsar is found to select from three different "modes" of emission, each corresponding to a different subpulse drift-rate. Transitions between these modes appear to follow certain simple rules of succession. A close resemblance to the pulsar PSR 0031-07 is noted, and a comparison with other pulsars suggests that the conventional definition of mode-changing might be reconsidered. We attempt to indicate the directions in which the polar cap model for pulsar emission must be developed if these observations are to be understood theoretically.
Fowler Lee A.
Wright Geoffrey A. E.
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