Image Details
Caption: Figure 9.
Posterior distributions and correlations of model parameters from the MCMC fit to the 2016 Vela glitch data, using the DD-ME2 interaction with L0 = 60 MeV. The anticorrelation between the preglitch slowdown duration Δt and magnitude Δνslow, and the anticorrelation between Vela mass M and entrainment strength, are clearly visible.
© 2026. The Author(s). Published by the American Astronomical Society.