Comparitive Study of Prole Stabilization in Slow, Fast and Millisecond Pulsars

Correlation methods are used to examine the prole stabilization of both normal and millisecond pulsars. A number of the pulsars stabilized in a characteristic manner that shows a \parabolic dependence|rationalizing earlier ndings that showed power-laws with two dieren t slopes. For the remaining objects, the distorting eects of mode changes or other prole dynamics are apparent in the correlations.