Author
Listed:
- Roland M. Crocker
(School of Physics, Monash University
Max-Planck-Institut für Kernphysik, PO Box 103980, Heidelberg, Germany)
- David I. Jones
(Max-Planck-Institut für Kernphysik, PO Box 103980, Heidelberg, Germany
School of Physics and Chemistry, University of Adelaide, North Terrace, South Australia 5005, Australia
Australia Telescope National Facility, Marsfield, New South Wales 2122, Australia)
- Fulvio Melia
(The Applied Math Program, and Steward Observatory, The University of Arizona, Tucson, Arizona 85721, USA)
- Jürgen Ott
(National Radio Astronomical Observatory, Charlottesville, PO Box O, 1003 Lopezville Road, Socorro, New Mexico 87801-0387, USA
California Institute of Technology, 1200 E. California Blvd, Caltech Astronomy, 105-24, Pasadena, California 91125, USA)
- Raymond J. Protheroe
(School of Physics and Chemistry, University of Adelaide, North Terrace, South Australia 5005, Australia)
Abstract
Centre of attraction There is ample evidence of a magnetic field near the centre of our Galaxy, but much uncertainty as to its strength. Estimates vary from the microgauss to the milligauss range — and values as great as 1,000 microgauss, about 10,000 times stronger than typical for the bulk of the Galaxy, have been reported. A new analysis of published radio and γ-ray data reveals a downward break in the region's non-thermal radio spectrum that suggests a Galactic Centre magnetic field of 50 microgauss or more. Taken with other evidence, the authors conclude that a field strength of about 100 microgauss is probable, on a par with that found in the inner regions of starburst galaxies.
Suggested Citation
Roland M. Crocker & David I. Jones & Fulvio Melia & Jürgen Ott & Raymond J. Protheroe, 2010.
"A lower limit of 50 microgauss for the magnetic field near the Galactic Centre,"
Nature, Nature, vol. 463(7277), pages 65-67, January.
Handle:
RePEc:nat:nature:v:463:y:2010:i:7277:d:10.1038_nature08635
DOI: 10.1038/nature08635
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