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CGPS studies of the Galactic Magnetic Field

Published online by Cambridge University Press:  05 March 2015

Joern Geisbuesch ,
R. Kothes  and
T. L. Landecker
Joern Geisbuesch
Affiliation:
DRAO, NSI-NRC, Penticton, V2A 6J9, Canada; email: [email protected]
R. Kothes
Affiliation:
DRAO, NSI-NRC, Penticton, V2A 6J9, Canada; email: [email protected]
T. L. Landecker
Affiliation:
DRAO, NSI-NRC, Penticton, V2A 6J9, Canada; email: [email protected]
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Abstract

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The Canadian Galactic Plane Survey (CGPS) is the largest effort of its kind to study and understand the Galactic Magnetic Field (GMF) and Interstellar Medium (ISM) in our Galaxy (see e.g. Taylor et al.2003). The CGPS has mapped the Galactic plane visible from DRAO on all spatial scales down to arcminute resolution in total intensity and polarized emission at νobs=1.4 GHz (see Landecker et al.2010). The latest results invoking Faraday rotation and polarization gradient studies of the CGPS are discussed.

Keywords

Radio continuum: ISMPolarizationISM: magnetic fieldsMethods: statistical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 393
Copyright
Copyright © International Astronomical Union 2015 

References

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Landecker, T., Reich, W., Reid, R., Reich, P., Wolleben, M., et al. 2010, A&A 520, 80Google Scholar
Taylor, A. R., Gibson, S., Peracaula, M., Martin, P., Landecker, T. L., et al. 2003, ApJ 125, 3145CrossRefGoogle Scholar