Speaker
Danai Antonopoulou
Description
Timing of neutron stars leads to information about their energy losses, magnetic field and internal dynamics including superfluid phenomena. In young pulsars, the long-term evolution of the spin-down rate can often be probed, in addition to irregularities such as timing noise and spin-up glitches. We will review the main observational attributes of their rotation and discuss some of the most recent results and how they shape our understanding of neutron star dynamics.
Author
Danai Antonopoulou
