MaNGA AGN dwarf galaxies (MAD)

Context. Feedback from an active galactic nucleus (AGN) is one of the most important mechanisms in galaxy evolution. This phenomenon is usually found in massive galaxies and is known to regulate star formation. Although dwarf galaxies are assumed to be regulated by supernova feedback, recent studies have offered evidence to support the presence of AGN outflows and feedback in dwarf galaxies. Aims. We investigate the presence of AGN outflows in a sample of 2292 dwarf galaxies with AGN signatures drawn from the MaNGA survey. Thanks to the integral field unit data from MaNGA, we are able to spatially resolve these outflows and study their kinematics and energetics. Methods. Using the Galaxy/AGN Emission Line Analysis TOol (GELATO) Python code, we fit the AGN-stacked spectrum of each galaxy. This is the stack of all the spaxels classified as AGNs or composites based on their emission line diagnostic diagrams and, in particular, the [OIII] λ 5007 Å emission line. If the galaxies exhibited a broad [OIII] emission line component in the stacked spectrum, we ran GELATO through all the spaxels classified as AGNs and composites in the emission line diagnostic diagrams. Results. We found 13 new dwarf galaxies that present outflow signatures based on the presence of a broad [OIII] emission line component. Their velocity measurement W 80 (width containing 80% of the flux of the [OIII] λ 5007 Å emission line) ranges from 205 to 566 km s −1 and the kinetic energy rate ranges from ∼10 35 to ∼10 39 erg s −1 . Stellar processes are unlikely to explain these outflow kinetic energy rates in the case of nine dwarf galaxies. We found a correlation between the W 80 velocity and the [OIII] luminosity as well as between the kinetic energy rate of the outflow and the bolometric luminosity spanning from massive to dwarf galaxies. This suggests a similar behaviour between the AGN outflows in the dwarf galaxy population and those in massive galaxies.