Cold molecular gas outflow encasing the ionized one in the Seyfert galaxy NGC 3281

We present ALMA CO(2-1) observations of the Seyfert 2 galaxy NGC 3281 at $\sim$ 100 pc spatial resolution. This was previously known to a bi-conical ionised gas outflow extending kpc from nucleus. The analysis CO moment and channel maps, as well kinematic modelling reveals two main components in molecular gas: one rotating plane another outflowing up 1.8 -- 2.6 nucleus, partially encasing component. mass component is $M_{\mathrm{mol},\mathrm{out}}$ = $(2.5\pm1.6){\times}10^{6}$ $\rm{M_{\odot}}$, representing 1.7 % total seen emission within inner 2.3 kpc. corresponding rate power are $\dot{M}_{\mathrm{mol},\mathrm{out}}$ 0.12 0.72 $\rm{M_{\odot} yr^{-1}}$ $\dot{E}_{\mathrm{mol},\mathrm{out}}$ (0.045 1.6) ${\times} 10^{40}$ $\rm{erg s^{-1}}$, which translates kinetic coupling efficiency with AGN only $10^{-4}$ 0.02 %. value reaches 0.1 when including both feedback gas, considering that part energy couples kinetically gas. Some non-rotating can also be attributed inflow towards similarity X-ray those other sources, suggests this may common property galactic outflows.