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An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102

Author

Listed:
  • D. Michilli

    (ASTRON, Netherlands Institute for Radio Astronomy
    Anton Pannekoek Institute for Astronomy, University of Amsterdam)

  • A. Seymour

    (National Astronomy and Ionosphere Center, Arecibo Observatory)

  • J. W. T. Hessels

    (ASTRON, Netherlands Institute for Radio Astronomy
    Anton Pannekoek Institute for Astronomy, University of Amsterdam)

  • L. G. Spitler

    (Max-Planck-Institut für Radioastronomie)

  • V. Gajjar

    (Space Science Laboratory, 7 Gauss Way, University of California
    Xinjiang Astronomical Observatory, CAS
    Key Laboratory of Radio Astronomy, Chinese Academy of Sciences)

  • A. M. Archibald

    (ASTRON, Netherlands Institute for Radio Astronomy
    Anton Pannekoek Institute for Astronomy, University of Amsterdam)

  • G. C. Bower

    (Academia Sinica Institute of Astronomy and Astrophysics)

  • S. Chatterjee

    (Cornell University, Ithaca)

  • J. M. Cordes

    (Cornell University, Ithaca)

  • K. Gourdji

    (Anton Pannekoek Institute for Astronomy, University of Amsterdam)

  • G. H. Heald

    (CSIRO Astronomy and Space Science)

  • V. M. Kaspi

    (McGill University)

  • C. J. Law

    (University of California)

  • C. Sobey

    (CSIRO Astronomy and Space Science
    International Centre for Radio Astronomy Research - Curtin University)

  • E. A. K. Adams

    (ASTRON, Netherlands Institute for Radio Astronomy
    Kapteyn Astronomical Institute, University of Groningen)

  • C. G. Bassa

    (ASTRON, Netherlands Institute for Radio Astronomy)

  • S. Bogdanov

    (Columbia Astrophysics Laboratory, Columbia University)

  • C. Brinkman

    (University of Vermont, Burlington)

  • P. Demorest

    (National Radio Astronomy Observatory)

  • F. Fernandez

    (National Astronomy and Ionosphere Center, Arecibo Observatory)

  • G. Hellbourg

    (University of California)

  • T. J. W. Lazio

    (Jet Propulsion Laboratory, California Institute of Technology)

  • R. S. Lynch

    (Green Bank Observatory
    Center for Gravitational Waves and Cosmology, Chestnut Ridge Research Building)

  • N. Maddox

    (ASTRON, Netherlands Institute for Radio Astronomy)

  • B. Marcote

    (Joint Institute for VLBI ERIC)

  • M. A. McLaughlin

    (Center for Gravitational Waves and Cosmology, Chestnut Ridge Research Building
    West Virginia University)

  • Z. Paragi

    (Joint Institute for VLBI ERIC)

  • S. M. Ransom

    (National Radio Astronomy Observatory)

  • P. Scholz

    (National Research Council of Canada, Herzberg Astronomy and Astrophysics, Dominion Radio Astrophysical Observatory)

  • A. P. V. Siemion

    (University of California
    Radboud University
    SETI Institute)

  • S. P. Tendulkar

    (McGill University)

  • P. Van Rooy

    (Case Western Reserve University)

  • R. S. Wharton

    (Max-Planck-Institut für Radioastronomie)

  • D. Whitlow

    (National Astronomy and Ionosphere Center, Arecibo Observatory)

Abstract

Polarimetric observations of the repeating fast radio burst source FRB 121102 suggest that the bursts may originate from a neutron star in the extreme magneto-ionic environment of an accreting massive black hole or supernova remnant.

Suggested Citation

  • D. Michilli & A. Seymour & J. W. T. Hessels & L. G. Spitler & V. Gajjar & A. M. Archibald & G. C. Bower & S. Chatterjee & J. M. Cordes & K. Gourdji & G. H. Heald & V. M. Kaspi & C. J. Law & C. Sobey &, 2018. "An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102," Nature, Nature, vol. 553(7687), pages 182-185, January.
  • Handle: RePEc:nat:nature:v:553:y:2018:i:7687:d:10.1038_nature25149
    DOI: 10.1038/nature25149
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