Figure 24 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 24.

Photon indices of the Crab pulsar in different phase ranges ("+"). The thick solid line represents the model prediction by the CRZ model (Zhang & Cheng 2002) and the dashed line represents the two-component model (Massaro et al. 2000).

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