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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. 1.

Electric structure in the gap. The solid line shows the solved accelerating field along the field line, which is located at 50% of the thickness from the last open field line. These results are for the inclination angle of 50° and for about 22% of the Goldreich‐Julian current in the gap. Beyond the null‐charge point, the dashed line is vacuum electric field obtained by Cheng et al. (1986a).

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