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Pulse Profiles, Spectra, and Polarization Characteristics of Nonthermal Emissions from the Crab‐like Pulsars

  • Authors: J. Takata and H.-K. Chang

Takata & Chang 2007 The Astrophysical Journal 670 677.

  • Provider: AAS Journals

Caption: Fig. 11.

Pulse profile in optical bands of PSR B0540−69. The result is for ﹩\alpha =30^{\circ }﹩ and ﹩\xi =98.5^{\circ }﹩. The top, middle, and bottom panels show the intensity, the position angle of the polarization, and the degree of the polarization, respectively.

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