Pulsar glitch substructure and pulsar interiors

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

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Solar and Stellar Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/216907

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0901.1495
 http://arxiv.org/abs/0901.1495

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arXiv