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Synchrotron Emission as a Tracer of the Outflow in M82

Published online by Cambridge University Press:  03 August 2017

E.R. Seaquist  and
Nils Odegard
E.R. Seaquist
Affiliation:
Department of Astronomy University of Toronto Toronto, Ontario M5S lAl, Canada
Nils Odegard
Affiliation:
General Sciences Corporation Goddard Space Flight Center Code 685.3, Greenbelt, MD 20771, U.S.A.

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 144: The Interstellar Disk-Halo Connection in Galaxies , 1991 , pp. 281 - 285
Copyright
Copyright © Kluwer 1991 

References

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