Figure 7 from X-Ray Phase-resolved Spectroscopy of PSRs B0531+21, B1509–58, and B0540

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X-Ray Phase-resolved Spectroscopy of PSRs B0531+21, B1509–58, and B0540–69 with RXTE

Authors: M. Y. Ge, F. J. Lu, J. L. Qu, S. J. Zheng, Y. Chen, and D. W. Han

Ge et al. 2012 The Astrophysical Journal Supplement Series 199 32.

Provider: AAS Journals

Caption: Figure 7.

Upper panel: the phase of the X-ray main peak of the Crab pulsar relative to the radio phase from the Jodrell Bank radio ephemeris, while the phase of the radio main peak is 1.0. Lower panel: the separation of the two X-ray peaks in different epochs.

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