BeppoSAX Observations of Crab-like Pulsars

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Scientific paper

We present a summary of the most important results obtained from BeppoSAX observations of Crab-like pulsars. Using the wide band (0.1 - 300 keV) covered by the scientific payload on board the mission it was possible to perform detailed spectral studies of this type of sources. An important result was that the spectra of the Crab pulsar, PSR B1509-58 and PSR B0540-69 are well described by log-parabolic laws with similar curvatures. For the Crab, in particular, we present the results phase resolved spectral analysis and give an interpretation of its pulsed emission as due to the superposition of two components.

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