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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. 10.

Left: Pulse profile in 10–20 keV bands for PSR B0540−69. The solid line is result for ﹩\alpha =30^{\circ }﹩ and ﹩\xi =98.5^{\circ }﹩ (and ﹩\xi =81.5^{\circ }﹩), and the dashed line is for ﹩\alpha =50^{\circ }﹩ and ﹩\xi =104^{\circ }﹩ (and ﹩\xi =76^{\circ }﹩). Right: Phase‐averaged spectrum of PSR B0540−69 for ﹩\alpha =30^{\circ }﹩ and ﹩\xi =98.5^{\circ }﹩ (and ﹩\xi =81.5^{\circ }﹩). The solid line represents the total emissions of the synchrotron radiation (dashed line) and the inverse‐Compton scattering (dotted line). The observation data are taken from de Plaa et al. (2003).

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