Pulsar glitch substructure and pulsar interiors

Details Pulsar glitch substructure and pulsar interiors Pulsar glitch substructure and pulsar interiors

2009-01-12

arxiv.org/abs/0901.1495v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Bursts, Pulses and Flickering: Wide-field monitoring of the dynamic radio sky, 2007

Scientific paper

Pulsar timing at the Mt Pleasant observatory focused on Vela, which could be tracked for 18 hours of the day. These nearly continuous timing records extend over 24 years allowing a great insight into details of timing noise, micro glitches and other more exotic effects. It has been found that the spin up for the Vela pulsar occurs instantaneously to within the uncertainties of the data. The potential for new, higher resolution data, to unveil insights of the Neutron Star interiors is discussed.

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