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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