26th of November 2015 |
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Emission-rotation correlation in pulsars: new discoveries with optimal techniques |
by Simon Johnston (CASS) |
Brook et al.
(2015) show that the profiles of radio pulsars can change with time and
that this change is accompanied by changes in the spin-down rate. The figure
above shows PSR J1602-5100 with the bottom panel showing the spin-down rate
and the middle panel show the profile evolution. Reference: Brook, P.R., Karastergiou, A., Johnston, S., Kerr, M., Shannon, R. M., Roberts, S.J. 2015, MNRAS, in press |