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Transient radio bursts from rotating neutron stars

Author

Listed:
  • M. A. McLaughlin

    (University of Manchester)

  • A. G. Lyne

    (University of Manchester)

  • D. R. Lorimer

    (University of Manchester)

  • M. Kramer

    (University of Manchester)

  • A. J. Faulkner

    (University of Manchester)

  • R. N. Manchester

    (Australia Telescope National Facility – CSIRO)

  • J. M. Cordes

    (Cornell University)

  • F. Camilo

    (Columbia University)

  • A. Possenti

    (INAF - Osservatorio Astronomico di Cagliari, Loc.)

  • I. H. Stairs

    (University of British Columbia)

  • G. Hobbs

    (Australia Telescope National Facility – CSIRO)

  • N. D'Amico

    (INAF - Osservatorio Astronomico di Cagliari, Loc.
    Universita di Cagliari, Strada Provinciale Monserrato-Sestu)

  • M. Burgay

    (INAF - Osservatorio Astronomico di Cagliari, Loc.)

  • J. T. O'Brien

    (University of Manchester)

Abstract

Pulsars: transient population A previously unknown population of superdense neutron stars has been identified. Termed RRATs, for rotating radio transients, their radio emissions vary on very short timescales, with bursts of 2 to 30 milliseconds occurring at intervals of 4 minutes to 3 hours. Eleven such objects have been found so far but their ephemeral nature suggests that there are many more in our Galaxy that remain unseen. This discovery implies a several-fold increase in the estimated radio-pulsar population, currently about 100,000.

Suggested Citation

  • M. A. McLaughlin & A. G. Lyne & D. R. Lorimer & M. Kramer & A. J. Faulkner & R. N. Manchester & J. M. Cordes & F. Camilo & A. Possenti & I. H. Stairs & G. Hobbs & N. D'Amico & M. Burgay & J. T. O'Brie, 2006. "Transient radio bursts from rotating neutron stars," Nature, Nature, vol. 439(7078), pages 817-820, February.
    • Handle: RePEc:nat:nature:v:439:y:2006:i:7078:d:10.1038_nature04440
    DOI: 10.1038/nature04440
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