The unusual glitch recoveries of the high magnetic field pulsar J1119$-$6127
D. Antonopoulou, P. Weltevrede, C.M. Espinoza, A.L. Watts, S., Johnston, R.M. Shannon, M. Kerr

TL;DR
This paper analyzes 16 years of radio timing data of pulsar J1119-6127, revealing ongoing spin-down evolution and linking glitch behavior to magnetar-like activity, with implications for neutron star evolution.
Contribution
It provides the first long-term analysis connecting glitch recovery peculiarities with magnetar-like properties in a high magnetic field pulsar.
Findings
Ongoing evolution of the spin-down rate observed.
No additional pulse profile variations detected.
Braking index measured at approximately 2.7, suggesting magnetar-like evolution.
Abstract
Providing a link between magnetars and radio pulsars, high magnetic field neutron stars are ideal targets to investigate how bursting/magnetospheric activity and braking torque variations are connected to rotational glitches. The last spin-up glitch of the highly magnetised pulsar J11196127 back in 2007 was the first glitch in a rotationally powered radio pulsar to be accompanied by radiative changes. Moreover, it was followed by an uncommon glitch relaxation that resulted in a smaller spin-down rate relative to the prediction of the pre-glitch timing model. Here, we present 4 years of new radio timing observations and analyse the total of 16 years of timing data for this source. The new data uncover an ongoing evolution of the spin-down rate, thereby allowing us to exclude permanent changes in the external or internal torque as a stand-alone cause of the peculiar features of the…
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