HEAD 2003 Meeting
Session 20. Magnetars and Young Neutron Stars III
Poster, Sunday-Wednesday, March 23, 2003, Duration of Meeting

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[20.09] A Radio Pulsar with an Ultra-High Magnetic Field

V. M. Kaspi (McGill University), M. A. McLaughlin (Jodrell Bank Observatory), I. H. Stairs (University of British Columbia), D. R. Lorimer, M. Kramer, A. G. Lyne (Jodrell Bank Observatory), R. N. Manchester (Australia Telescope National Facility), F. Camilo (Columbia University), G. Hobbs (Jodrell Bank Observatory), A. Possenti (Osservatorio Astronomico di Bologna), N. D'Amico (Universita degli Studi di Cagliari), A. J. Faulkner (Jodrell Bank Observatory)

We report the discovery of PSR J1847-0130, a young radio pulsar with a spin period 6.7 s and an inferred surface dipolar magnetic field of 9.4 x 1013 G. This pulsar's period, second largest among radio pulsars, and magnetic field, highest among all known radio pulsars, are indistinguishable from those of some Anomalous X-ray Pulsars, which are known to be magnetars. This discovery proves that inferred magnetic field cannot be the sole parameter determining whether a neutron star will exhibit magnetar-like properties. This discovery creates new challenges for understanding the emission mechanisms of and the relationship between these two manifestations of young neutron stars.

The author(s) of this abstract have provided an email address for comments about the abstract: mclaughl@jb.man.ac.uk

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Bulletin of the American Astronomical Society, 35#2
© 2003. The American Astronomical Soceity.