Pulsar glitch substructure and pulsar interiors

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dc.creatorDodson, R.
dc.creatorDeshpande, A.
dc.creatorLewis, D.
dc.creatorMcCulloch, P.
dc.date2009-01-12
dc.date.accessioned2026-07-07T12:32:48Z
dc.date.available2026-07-07T12:32:48Z
dc.descriptionPulsar 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.
dc.descriptionBursts, Pulses and Flickering: Wide-field monitoring of the dynamic radio sky, 2007
dc.identifierhttps://arxiv.org/abs/0901.1495
dc.identifierhttp://arxiv.org/abs/0901.1495
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216907
dc.subjectSolar and Stellar Astrophysics
dc.titlePulsar glitch substructure and pulsar interiors
dc.typetext

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