Image Details
Caption: Figure 2.
Distribution histograms of the surface magnetic field (﹩\mathrm{log}{B}_{p}﹩) and the initial rotation period (﹩\mathrm{log}{P}_{0}﹩) for magnetars, with Gaussian fits, under the assumption of an X-ray conversion efficiency of 0.5.
© 2026. The Author(s). Published by the American Astronomical Society.