Pulsar timing noise from superfluid turbulence
Andrew Melatos, Bennett Link
Monthly Notices of the Royal Astronomical Society | OXFORD UNIV PRESS | Published : 2014
Awarded by USA National Science Foundation
Awarded by NASA
The authors thank V. Ravi, G. Hobbs, W. Coles, R. Shannon and R. Manchester for stimulating discussions and for preparing the observational data plotted in the figures. The power spectral density curves for PSR J1909-3744 and PSR J1939+2134 in Fig. 1 are provided by the Parkes Pulsar Timing Array Project and have been published in fig. 11 of Manchester et al. ( 2013). This research was supported by the Australian Research Council and the USA National Science Foundation (Award AST-1211391), and by NASA (Award NNX12AF88G).