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CO Observations of a Region with Strong Polarization in M31
Published online by Cambridge University Press: 19 July 2016
Abstract
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
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