<scp>CO</scp> kinematics unveil outflows plausibly driven by a young jet in the gigahertz peaked radio core of <scp>NGC 6328</scp>

We report the detection of outflowing molecular gas in center nearby (z=0.014) massive radio galaxy NGC6328. The core galaxy, PKS B1718-649, is identified as a Gigahertz Peaked Spectrum source with compact (2 pc) double lobe morphology. used ALMA CO(2-1) and CO(3-2) observations at 100 pc resolution to study kinematics up ~5 kpc from center. While bulk settled highly warped disk, inner 300 disk along orientation jet, we high-excitation high-velocity that cannot be attributed any regular kinematic component based on our detailed 3D modeling data. dispersion also suggests it not part an inflowing, shredding structure. These results suggest presence outflow 3 8 solar masses per year. possibly originated interaction jet dense interstellar medium, even though emission detected closer than outflow. In this sense, resembles NGC1377, 4C31.04 ESO420-G13, which outflows are linked faint or past activity.