text: 176,18,1278122949988569089,1186047738607263744,Rogemar A Riffel,"New paper on arXiv: <LINK> Providing observational constraints in the multi-phase gas kinematics on 10-100 pc scales of galaxies is fundamental to better understand the role feedback from Active Galactic Nuclei (AGN) in the evolution of galaxies. We use Gemini NIFS to map de hot molecular and ionized gas kinematics in the inner 500 pc of NGC1275, the brightest galaxy of the Perseus cluster. <LINK> From the fitting of the CO absorption bandheads in the K-band, we derive a stellar velocity dispersion of  ~265  km/s , which implies a black hole mass of  ~1.1E9 solar masses. <LINK> The gas kinematics present two components, one (narrow) due to gas at velocities close to the systemic velocity of the galaxy and another (broad) due to outflows produced by the central active nucleus. <LINK> We find hot (T&gt; 1000 K) molecular and ionized outflows with velocities of up to 2000 km/s and mass outflow rates of 2.7E-2 solar masses/year and 1.6 solar masses/year, respectively in each of these gas phases. The kinetic power of the ionized outflows corresponds to only 0.05% of the luminosity of the AGN of NGC 1275, indicating that they are not powerful enough to provide significant AGN feedback, but may be effective in redistributing the gas in the central region of the galaxy. The H2 and [FeII] emission is produced mainly by shocks produced by the AGN winds, as revealed by the emission-line ratio diagnostic diagram and the observed kinematics. <LINK> My collaborators in this work are @thaisa_sb (UFRGS), Nadia Zakamska (JHU) and @RiffelRogerio (UFRGS). @venkatessh Thanks! Indeed, the ALMA data of NGC1275 were already published by Nagai et al. The ALMA CO maps show the compact molecular disk (&lt;100 pc), but not the outflow. Definitely, we should talk about ALMA data for some nearby Seyferts that we have NIFS data...",https://arxiv.org/abs/2006.15198,"The role of feedback from Active Galactic Nuclei (AGN) in the evolution of galaxies is still not not fully understood, mostly due to the lack of observational constraints in the multi-phase gas kinematics on the ten to hundred parsec scales. We have used the Gemini Near-infrared Integral Field Spectrograph (NIFS) to map the molecular and ionized gas kinematics in the inner 900$\times$900 pc$^2$ of the Seyfert galaxy NGC1275 at a spatial resolution of $\sim$70 pc. From the fitting of the CO absorption bandheads in the 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 with velocities 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 ionized outflows corresponds to only 0.05 per cent of the luminosity of the AGN of NGC 1275, indicating that they are not powerful enough to provide significant AGN feedback, but may be effective in redistributing the gas in the central region of the galaxy. The AGN driven outflows seem to be responsible for the shocks necessary to produce the observed H$_2$ and [Fe II] line emission. ",Ionized and hot molecular outflows in the inner 500 pc of NGC1275,9,"['New paper on arXiv:\xa0<LINK>\nProviding observational constraints in the multi-phase gas kinematics on 10-100 pc scales of galaxies is fundamental to better understand the role feedback from Active Galactic Nuclei (AGN) in the evolution of galaxies.', 'We use Gemini NIFS to map de hot molecular and ionized gas kinematics in the inner 500 pc of NGC1275, the brightest galaxy of the Perseus cluster. https://t.co/48wCobXBRQ', 'From the fitting of the CO absorption bandheads in the K-band, we derive a stellar velocity dispersion of\xa0 ~265\xa0 km/s , which implies a black hole mass of\xa0 ~1.1E9 solar masses. https://t.co/VHASWFxqW3', 'The gas kinematics present\xa0two components, one (narrow) due to gas at velocities close to the systemic\xa0velocity of the galaxy and another (broad) due to outflows produced by the central active nucleus. https://t.co/Mpna6Hn0sY', 'We find hot (T&gt; 1000 K) molecular and ionized outflows with velocities of up to 2000 km/s and mass outflow rates of 2.7E-2 solar masses/year and 1.6 solar masses/year, respectively in each of these gas phases.', 'The kinetic power of the ionized outflows corresponds to only 0.05% of the luminosity of the AGN of NGC 1275, indicating that they are not powerful enough to provide significant AGN feedback, but may be effective in redistributing the gas in the central region of the galaxy.', 'The H2 and [FeII] emission is produced mainly by shocks produced by the AGN winds, as revealed by the emission-line ratio diagnostic diagram and the observed kinematics. https://t.co/AZ8M83ezco', 'My collaborators in this work are @thaisa_sb (UFRGS),  Nadia Zakamska (JHU) and @RiffelRogerio (UFRGS).', '@venkatessh Thanks! Indeed, the ALMA data of NGC1275 were already published by Nagai et al. The ALMA CO maps show the compact molecular disk (&lt;100 pc), but not the outflow. Definitely, we should talk about ALMA data for some nearby Seyferts that we have NIFS data...']",20,06,1832