![]() ![]() ![]() Second, we find definitive evidence for a rotational-frequency overshoot and fast relaxation following the glitch. First, we constrain the glitch rise time to less than 12.6 s with 90% confidence, almost three-times shorter than the previous best constraint. We fit models of the star’s rotation frequency to the pulsar data, and present the following three results. ![]() The 2016 Vela glitch observed by the Mount Pleasant radio telescope provides the first opportunity to study pulse-to-pulse dynamics of a pulsar glitch, opening up new possibilities to study the neutron star’s interior. ![]()
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