Chen, SinaSinaChenLaor, AriAriLaorBehar, EhudEhudBeharBALDI, Ranieri DiegoRanieri DiegoBALDIGelfand, Joseph D.Joseph D.GelfandKimball, Amy E.Amy E.KimballMcHardy, Ian M.Ian M.McHardyOrosz, GaborGaborOroszParagi, ZsoltZsoltParagi2025-01-022025-01-0220240004-637Xhttp://hdl.handle.net/20.500.12386/35597Does a broad-line region (BLR) wind in radio-quiet (RQ) active galactic nuclei (AGN) extend to parsec scales and produce radio emission? We explore the correlations between a parsec-scale radio wind and the BLR wind in a sample of 19 RQ Palomar-Green quasars. The radio wind is defined based on the spectral slope and the compactness of the emission at 1.5-5 GHz, and the BLR wind is defined by the excess blue wing in the C iv emission line profile. The five objects with both radio and BLR wind indicators are found at high Eddington ratios, L/L Edd (≥0.66), and eight of the nine objects with neither radio nor BLR winds reside at low L/L Edd (≤0.28). This suggests that the BLR wind and the radio wind in RQ AGN are related to a radiation-pressure-driven wind. Evidence for free-free absorption by AGN photoionized gas, which flattens the spectral slope, is found in two objects. Radio outflows in three low-L/L Edd (0.05-0.12) objects are likely from a low-power jet, as suggested by additional evidence. The presence of a mild equatorial BLR wind in four intermediate-L/L Edd (0.2-0.4) objects can be tested with future spectropolarimetry.STAMPAenArticle10.3847/1538-4357/ad74fc2-s2.0-85207715274https://iopscience.iop.org/article/10.3847/1538-4357/ad74fchttps://api.elsevier.com/content/abstract/scopus_id/85207715274FIS/05 - ASTRONOMIA E ASTROFISICA