Exposing Drifting Subpulses from the Slowest to the Fastest Pulsars.

Details Exposing Drifting Subpulses from the Slowest to the Fastest Pulsars. Exposing Drifting Subpulses from the Slowest to the Fastest Pulsars.

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.0405v&link_type=abstract

American Astronomical Society Meeting 208, #4.05; Bulletin of the American Astronomical Society, Vol. 38, p.82

Astronomy and Astrophysics

Astronomy

Scientific paper

Pulsar emission is surprisingly similar over a vast range of periods and magnetic fields: all the way from the 2-millisecond 108-G recycled pulsars to the 6-second 1014-G magnetar-like regular pulsars. We think the stability and speed of the subpulse drift seen over this whole range can discern between different mechanisms for pulsar emission. Using two new techniques to discern and interpret subpulse drift patterns in both dim and bright pulsars, we investigate the relation between subpulse-drift speed and the pulsar period and magnetic field.

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