High resolution polarimetry of the inner Galaxy
arXiv:astro-ph/0111114 · doi:10.1063/1.1471818
Abstract
We present our results from the Southern Galactic Plane Survey, an effort to map the fourth quadrant of the Milky Way in linear polarization at a frequency of 1.4 GHz and at a resolution of 1-2 arcmin. These data are a powerful probe of both the turbulence and large-scale structure of magneto-ionic gas, and have revealed a variety of new features in the interstellar medium.
9 pages, 3 embedded EPS figures. To appear in "Astrophysical Polarized Backgrounds", eds Cecchini et al, AIP Conference Proceedings, in press