Polarization Structures in the Canadian Galactic Plane Survey: A Multispectral View

Details Polarization Structures in the Canadian Galactic Plane Survey: A Multispectral View Polarization Structures in the Canadian Galactic Plane Survey: A Multispectral View

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mim..proc...33k&link_type=abstract

The Magnetized Interstellar Medium, Proceedings of the conference, held in Antalya, Turkey, September 8 - 12, 2003, Eds: B. Uyan

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Scientific paper

The comparison of structures, linearly polarized at 1420 MHz, with images in Stokes I, observations at other frequencies, and other sources can help us to learn more about the nature of these objects. We can distinguish between actual emission structures and those that merely affect the smooth background polarization by Faraday Rotation, the so-called Faraday screens. We can also gain more information about electron density and/or magnetic field enhancements that cause the Faraday Rotation and the distances to these objects.

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