Outflow kinematics manifested by the H-alpha line: gas outflows in Type 2 AGNs. IV
arXiv:1707.05895 · doi:10.3847/1538-4357/aa80e8
Abstract
Energetic ionized gas outflows driven by active galactic nuclei (AGN) have been studied as a key phenomenon related to AGN feedback. To probe the kinematics of the gas in the narrow line region, [O III] 5007 has been utilized in a number of studies, showing non-virial kinematic properties due to AGN outflows. In this paper, we statistically investigate whether the H-alpha emission line is influenced by AGN driven outflows, by measuring the kinematic properties based on the H-alpha line profile, and by comparing them with those of [O III]. Using the spatially integrated spectra of ~37,000 Type 2 AGNs at z < 0.3 selected from the SDSS DR7, we find a non-linear correlation between H-alpha velocity dispersion and stellar velocity dispersion, which reveals the presence of the non-gravitational component, especially for AGNs with a wing component in H-alpha. The large H-alpha velocity dispersion and velocity shift of luminous AGNs are clear evidence of AGN outflow impacts on hydrogen gas, while relatively smaller kinematic properties compared to those of [O III] imply that the observed outflow effect on the H-alpha line is weaker than the case of [O III].
References in corpus (8)
- The Host Galaxies and Classification of Active Galactic Nuclei
- A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
- Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
- The black hole mass - stellar velocity dispersion relation of narrow-line Seyfert 1 galaxies
- Radiative pressure feedback by a quasar in a galactic bulge
- The Limited Impact of Outflows: Integral-Field Spectroscopy of 20 Local AGNs
- A Census of Gas Outflows in Type 2 Active Galactic Nuclei
- Misclassified type 1 AGNs in the local universe
Cited by in corpus (11)
- KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at -
- Fast Outflows in Hot Dust-Obscured Galaxies with Keck/NIRES
- Spectral Classification and Ionized Gas Outflows in WISE-Selected Hot Dust-Obscured Galaxies
- Ionized Outflows in Nearby Quasars are Poorly Coupled to their Host Galaxies
- The Dust-to-Gas Ratio and the Role of Radiation Pressure in Luminous, Obscured Quasars
- Tracing the outflow kinematics in Type 2 Active Galactic Nuclei
- A Chandra study of Abell 795 -- a sloshing cluster with a FR0 radio galaxy at its center
- Unraveling the complex structure of AGN-driven outflows: V. Integral-field spectroscopy of 40 moderate-luminosity Type-2 AGNs
- Unraveling the complex structure of AGN-driven outflows: IV. Comparing AGNs with and without strong outflows
- Discovery of a Low-Redshift Hot Dust-Obscured Galaxy
- An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole