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The role of feedback from Active Galactic Nuclei (AGN) in the evolution ofgalaxies is still not not fully understood, mostly due to the lack ofobservational constraints in the multi-phase gas kinematics on the ten tohundred parsec scales. We have used the Gemini Near-infrared Integral FieldSpectrograph (NIFS) to map the molecular and ionized gas kinematics in theinner 900$\times$900 pc$^2$ of the Seyfert galaxy NGC1275 at a spatialresolution of $\sim$70 pc. From the fitting of the CO absorption bandheads inthe K-band, we derive a stellar velocity dispersion of $265\pm26$ km s$^{-1}$,which implies a black hole mass of $M_{\rm SMBH}=1.1^{+0.9}_{-0.5}\times10^9$M$_\odot$. We find hot ($T\gtrsim1000$ K) molecular and ionized outflows withvelocities of up to 2 000 km s$^{-1}$ and mass outflow rates of$2.7\times10^{-2} {\rm M_\odot}$ yr$^{-1}$ and $1.6 {\rm M_\odot}$ yr$^{-1}$,respectively, in each of these gas phases. The kinetic power of the ionizedoutflows corresponds to only 0.05 per cent of the luminosity of the AGN of NGC1275, indicating that they are not powerful enough to provide significant AGNfeedback, but may be effective in redistributing the gas in the central regionof the galaxy. The AGN driven outflows seem to be responsible for the shocksnecessary to produce the observed H$_2$ and [Fe II] line emission.

Ionized and hot molecular outflows in the inner 500 pc of NGC1275