Figure 19 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 19.

X-ray profiles of PSR B0540−69 in different energy ranges. The two dot-dashed lines represent the two Gaussian components used to fit the pulses. The thin and thick dashed lines represent the model results from Zhang & Cheng (2000) and Takata & Chang (2007) separately.

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