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We present results from a combined radio polarization and emission line studyof five type 2 quasars at $z<0.2$ with the Karl G. Jansky Very Large Array(VLA) B-array at 5 GHz and Hubble Space Telescope (HST) [O III] observations.These five sources are known to exhibit close association between radiostructures and ionized gas morphology and kinematics. Four sources (J0945+1737,J1000+1242, J1356+1026 and J1430+1339) show polarization in the current data.J1010+1413 is the unpolarized source in our sample. We detect $0.5-1\%$fractional polarization in the radio cores and a high fractional polarization($10-30\%$) in the lobes of these sources. The morphological, spectral andpolarization properties suggest a jet origin for radio emission in J0945+1737,J1000+1242, J1010+1413 and J1430+1339 whereas the current data cannot fullydiscern the origin of radio emission (jet or wind) in J1356+1026. Ananti-correlation between various polarized knots in the radio and [O III]emission is observed in our sources, similar to that observed in someradio-loud AGN in the literature. This suggests that the radio emission islikely to be depolarized by the emission-line gas. By modeling thedepolarization effects, we estimate the size of the emission-line gas clouds tobe $\sim(2.8\pm1.7)\times10^{-5}$ parsec and the amount of thermal materialmixed with the synchrotron plasma to be$\sim(1.01\pm0.08)\times10^{6}$M$_\odot$ in the lobe of J0945+1737 (whichexhibits the most prominent polarization signature in its lobe). The currentwork demonstrates that the interplay of jets/winds and emission-line gas ismost likely responsible for the nature of radio outflows in radio-quiet AGN.

The Quasar Feedback Survey: Revealing the Interplay of Jets, Winds & Emission Line Gas in Type 2 Quasars with Radio Polarization