Correlation Between Accretion Torque and Accretion Rate in KS 1947+300

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We have applied the analysis technique we have previously applied to other transient X-ray pulsars (GRO J1744-28 and SAX J2103.5+4545) to KS 1947+300. We have made precise measurements of the changes in the pulse period and of the observed X-ray flux. We have correlated the flux and torque measurements to use this source as a test of binary accretion theory. This source, the only accreting X-ray pulsar to display clear evidence of a glitch provides a unique opportunity to explore how glitches might relate to regular steady accretion.

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