Author
Listed:
- R. P. Eatough
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- H. Falcke
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
ASTRON, PO Box 2, 7990 AA Dwingeloo, The Netherlands)
- R. Karuppusamy
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- K. J. Lee
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- D. J. Champion
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- E. F. Keane
(Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK)
- G. Desvignes
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- D. H. F. M. Schnitzeler
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- L. G. Spitler
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- M. Kramer
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK)
- B. Klein
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
Bonn-Rhein-Sieg University of Applied Sciences, Grantham-Allee 20, D-53757 Sankt Augustin, Germany)
- C. Bassa
(Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK)
- G. C. Bower
(B-20 Hearst Field Annex, University of California)
- A. Brunthaler
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- I. Cognard
(LPC2E/CNRS - Université d’Orléans, 45071 Orléans, France
Nançay/Paris Observatory, 18330 Nançay, France)
- A. T. Deller
(ASTRON, PO Box 2, 7990 AA Dwingeloo, The Netherlands)
- P. B. Demorest
(National Radio Astronomy Observatory, 520 Edgemont Road)
- P. C. C. Freire
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- A. Kraus
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- A. G. Lyne
(Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK)
- A. Noutsos
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
- B. Stappers
(Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK)
- N. Wex
(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany)
Abstract
The unusually large Faraday rotation of a newly discovered pulsar indicates that there is a dynamically important magnetic field near the supermassive black hole believed to lie at the centre of the Milky Way.
Suggested Citation
R. P. Eatough & H. Falcke & R. Karuppusamy & K. J. Lee & D. J. Champion & E. F. Keane & G. Desvignes & D. H. F. M. Schnitzeler & L. G. Spitler & M. Kramer & B. Klein & C. Bassa & G. C. Bower & A. Brun, 2013.
"A strong magnetic field around the supermassive black hole at the centre of the Galaxy,"
Nature, Nature, vol. 501(7467), pages 391-394, September.
Handle:
RePEc:nat:nature:v:501:y:2013:i:7467:d:10.1038_nature12499
DOI: 10.1038/nature12499
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