Two Radio Pulsars with Magnetar Fields

@inproceedings{Mclaughlin2003TwoRP,
  title={Two Radio Pulsars with Magnetar Fields},
  author={Maura Mclaughlin and Victoria M. Kaspi and Ingrid H. Stairs and Duncan R. Lorimer and Andrew G. Lyne and Michael Kramer and Richard N. Manchester and Andrew J. Faulkner and George Hobbs and F. Camilo and A. PossentiN. D'Amico},
  year={2003}
}
PSRs J1847-0130 and J1718-37184 have inferred surface dipole magnetic fields greater than those of any other known pulsars and well above the ``quantum critical field'' above which some models predict radio emission should not occur.These fields are similar to those of the anomalous X-ray pulsars (AXPs), which growing evidence suggests are ``magnetars''. The lack of AXP-like X-ray emission from these radio pulsars (and the non-detection of radio emission from the AXPs) creates new challenges… Expand

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