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Golden, A,Shearer, A,Beskin, G,Kramer, M,Wex, N,Wielebinski, R
PULSAR ASTRONOMY - 2000 AND BEYOND: IAU COLLOQUIUM 177
Unpulsed optical emission from the Crab pulsar
2000
February
Published
1
()
Optional Fields
Kramer
297
298
Using the high speed 2-d TRIFFID photometer, we have obtained phase resolved photometry of the Crab pulsar in UBV that allows us to flux the unpulsed light curve component. Following de-extinction, weighted least-square fitting indicates a power-law exponent of alpha = -0.62 +/- 0.49. This is steeper than that reported for the peak components and its origin remains unclear with respect to contemporary magnetospheric theory.
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