Figure 2 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 2.

X-ray profiles of the Crab pulsar in different energy ranges. Phase 0 represents the position of the main radio peak. The dashed line represents the result of the theoretical model (Jia et al. 2007).

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