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

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...2e..63v&link_type=abstract

On the Present and Future of Pulsar Astronomy, 26th meeting of the IAU, Joint Discussion 2, 16-17 August, 2006, Prague, Czech Re

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 10^8 G recycled
pulsars to the 6-second 10^14 G magnetar-like regular pulsars. We
investigate how the curious instabilities called 'drifting subpulses' we
observe can discern between different mechanisms for pulsar emission.

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