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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 8.

Left panel: the distribution of the phase lag between the X-ray main peak and the radio main peak of the Crab pulsar with bin size 5.8 × 10 −4 periods. The dashed line represents the fitted Gaussian function with μ = −0.0101 and σ = 1.3 × 10 −3. Right panel: the distribution of the separation between the two X-ray peaks with bin size 9.6 × 10 −5 periods. The dashed line represents the fitted Gaussian function with μ = 0.4005 and σ = 2.5 × 10 −4.

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