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We present a study of molecular gas, traced via CO (3-2) from ALMA data, offour z< 0.2, `radio quiet', type 2 quasars (log [L(bol)/(erg/s)] = 45.3 - 46.2;log [L(1.4 GHz)/(W/Hz)] = 23.7 - 24.3). Targets were selected to have extendedradio lobes (>= 10 kpc), and compact, moderate-power jets (1 - 10 kpc; log[Pjet/(erg/s)]= 43.2 - 43.7). All targets show evidence of central molecularoutflows, or injected turbulence, within the gas disks (traced viahigh-velocity wing components in CO emission-line profiles). The inferredvelocities (Vout = 250 - 440 km/s) and spatial scales (0.6 - 1.6 kpc), areconsistent with those of other samples of luminous low-redshift AGN. In twotargets, we observe extended molecular gas structures beyond the central disks,containing 9 - 53 % of the total molecular gas mass. These structures tend tobe elongated, extending from the core, and wrap-around (or along) the radiolobes. Their properties are similar to the molecular gas filaments observedaround radio lobes of, mostly `radio loud', Brightest Cluster Galaxies. Theyhave: projected distances of 5 - 13 kpc; bulk velocities of 100 - 340 km/s;velocity dispersion of 30 - 130 km/s; inferred mass outflow rates of 4 - 20Msolar/yr; and estimated kinetic powers of log [Ekin/(erg/s)]= 40.3 - 41.7. Ourobservations are consistent with simulations that suggest moderate-power jetscan have a direct (but modest) impact on molecular gas on small scales, throughdirect jet-cloud interactions. Then, on larger scales, jet-cocoons can push gasaside. Both processes could contribute to the long-term regulation of starformation.

Quasar Feedback Survey: molecular gas affected by central outflows and by ~10 kpc radio lobes reveal dual feedback effects in `radio quiet' quasars