Image Details
Caption: Figure 11.
Comparison between the measured eccentricity and the expected eccentricity, as predicted by E. S. Phinney (1992), for PSR J0125−5854 (as a cross) and the 12 pulsars likely with WD companions. The solid line is where the measured and expected eccentricities are equal, and the dashed lines are where the measured and expected eccentricities differ by a factor of 2.
© 2026. The Author(s). Published by the American Astronomical Society.