Looking at radio-quiet AGN with radio polarimetry

The dominant radio emission mechanism in radio-quiet quasars (RQQs) is an open question. Primary contenders include: low-power jets, winds, star-formation and coronal emission. Our work suggests that polarization emission-line studies can help to distinguish between these scenarios determine the primary contributor. multi-frequency, multi-scale study has revealed a composite jet "wind" outflow radio-intermediate quasar, III Zw 2, as well BALQSO, Mrk 231. conjunction with [O III] of five type 2 RQQs have provided insights on interplay jets/winds gas. These sources reveal anti-correlation polarized This similar observed some radio-loud active galactic nuclei (AGN) literature could be depolarized by Overall, our close interaction surrounding gaseous environment likely responsible for their stunted form RQ RI AGN.