161 citations · 306 across the 7 of their papers we have counts for
8 papers
Pulsar glitch substructure and pulsar interiors
R. Dodson, A. Deshpande, D. Lewis +1
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…
Two decades of pulsar timing of Vela
Richard Dodson, Dion Lewis, Peter McCulloch
Pulsar timing at the Mt Pleasant observatory has focused on Vela, which can be tracked for 18 hours of the day. These nearly continuous timing records extend over 24 years allowing…
The Vela pulsar, the key?
Richard Dodson, Dion Lewis, David Legge +4
Of all pulsars known Vela has been one of the most productive in terms in understanding pulsars and their characteristics. We present the latest results derived from Australian tel…
The Vela Pulsar's Radio Nebula
R. Dodson, D. Lewis, D. McConnell +1
We have discovered that the radio nebula surrounding the Vela pulsar covers a much wider extent than previously reported, with two lobes to the North and South of the pulsar. Indic…
Pulsar observations at Mt. Pleasant
D. R. Lewis, R. G. Dodson, P. D. Ramsdale +1
Two daily pulsar monitoring programs are progressing at the Mount Pleasant Observatory, Hobart, Tasmania, Australia. A new system involving the 26-metre radio telescope monitors 10…
High time resolution observations of the January 2000 glitch in the Vela pulsar
R. G. Dodson, P. M. McCulloch, D. R. Lewis
Pulsars are rotating neutron stars, sweeping the emission regions from the magnetic poles across our line of sight. Isolated neutron stars lose angular momentum through dipole radi…