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CO Observations of a Region with Strong Polarization in M31

Published online by Cambridge University Press:  19 July 2016

E. Bajaja ,
E.M. Berkhuijsen  and
R. Beck
E. Bajaja
Affiliation:
1 Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, D–5300 Bonn 1, F.R.G. 2 Instituto Argentino de Radioastronomia, C.C. 5, Villa Elisa (1894), Argentina
E.M. Berkhuijsen
Affiliation:
1 Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, D–5300 Bonn 1, F.R.G.
R. Beck
Affiliation:
1 Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, D–5300 Bonn 1, F.R.G.

Abstract

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A region with strong radio polarization in the SW of M31 was observed in the 12CO(1–0) line. The results are compared with the radio continuum, HI and Ha. The CO emission appears to be correlated with the total radio emission, but anticorrelated with the polarized intensity.

Type
5. The Polarization, Magnetic Field and Velocity Structure of External Spiral Galaxies
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 203 - 204
Copyright
Copyright © Kluwer 1990 

References

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