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Synchrotron Emission as a Tracer of the Outflow in M82
Published online by Cambridge University Press: 03 August 2017
Abstract
We report the discovery of radio synchrotron emission from the outflow in M82. The brightness morphology and radio spectral index distribution add new insights into the physical processes and origin of the wind, which are briefly discussed in this paper.
- Type
- II. The Disk-Halo Interface in Other Galaxies
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- Copyright © Kluwer 1991