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AbstractRecently, PSR J0738-4042 has grown a bright new emission component in its average pulse profile. Using data from Parkes and HartRAO, spanning back to the early 1980s, and applying statistical techniques to model the pulse profile shape with time, we have uncovered unexpected long-term variability, which is very well correlated with changes in the spin-down rate. We present these findings in the context of a growing population of radio-variable pulsars with correlated timing irregularities, including the intermittent pulsars, state-changing pulsars and other individual examples.

Original publication

DOI

10.1017/s1743921312023496

Type

Journal article

Journal

Proceedings of the International Astronomical Union

Publisher

Cambridge University Press (CUP)

Publication Date

08/2012

Volume

8

Pages

161 - 161