CO kinematics unveil outflows plausibly driven by a young jet in the gigahertz peaked radio core of NGC 6328
We report the detection of outflowing molecular gas in the center of the nearby (z = 0.014) massive radio galaxy NGC 6328. The radio core of the galaxy, PKS B1718-649, is identified as a gigahertz peaked spectrum source with a compact (2 pc) double radio lobe morphology. We used ALMA CO(2-1) and CO(3-2) observations at 100 pc resolution to study
Papachristou, Michalis et al.
Advertised on:
11
2021