The nuclear region of NGC 613 -- II. Kinematics and stellar archaeology
arXiv:2006.09571 · doi:10.1093/mnras/staa1500
Abstract
In this work, we continue the study of the central region of NGC 613 by da Silva et al. (2020), by analysing the stellar and gas kinematics and the stellar archaeology in optical and near-infrared data cubes. The high spatial resolution of the Gemini Multi-Object Spectrograph (GMOS) data cube allowed the detection, using spectral synthesis methods, of an inner circumnuclear ring, with a radius of 1 arcsec, composed of 10-yr stellar populations. Such a ring is located between the nucleus and the circumnuclear ring composed by H II regions detected in previous works. Besides that, there is a stellar rotation around the nucleus and the rings follow the same direction of rotation with different velocities. The intensity-weighted average stellar velocity dispersion at the centre is 92 3 km s. Three distinct gas outflow components were detected. The direction of the outflow observed with the H emission line is compatible with the direction of the previously observed radio jet. The direction of one of the outflows detected in the [O III]5007 emission coincides with the axis of the ionization cone. There is no difference regarding the stellar populations and the stellar kinematics along the double stellar emission, probably separated by a dust lane as mentioned in Paper I, confirming that they are part of the same structure.
arXiv comment17 pages, 17 figures
References in corpus (27)
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- Parametric Recovery of Line-of-Sight Velocity Distributions from Absorption-Line Spectra of Galaxies via Penalized Likelihood
- MILES: A Medium resolution INT Library of Empirical Spectra
- The 1000 Brightest HIPASS Galaxies: HI Properties
- How Do Massive Black Holes Get Their Gas?
- The subarcsecond mid-infrared view of local active galactic nuclei: II. The mid-infrared--X-ray correlation
- ALMA observations of molecular tori around massive black holes
- Observational Constraints on the Feeding of Supermassive Black Holes
- Hubble flow around Fornax cluster of galaxies
- A SINFONI view of Galaxy Centers: Morphology and Kinematics of five Nuclear Star Formation Rings
- A Connection between Star Formation in Nuclear Rings and their Host Galaxies
- The Gemini spectral library of near-IR late type stellar templates and its application for velocity dispersion measurements
- Fueling AGN-I: How the Global Characteristics of the Central Kiloparsec of Seyferts differ from Quiescent Galaxies
- ALMA captures feeding and feedback from the active galactic nucleus in NGC613
- Dissecting Galaxies: Separating Star Formation, Shock Excitation and AGN Activity in the Central Region of NGC 613
- A treatment procedure for Gemini North/NIFS data cubes: application to NGC 4151
- New Compton-thick AGN in the circumnuclear water maser hosts UGC3 789 and NGC 6264
- The circumnuclear environment of NGC613: a nuclear starburst caught in the act?
- A treatment procedure for VLT/SINFONI data cubes: application to NGC 5643
- Are (pseudo)bulges in isolated galaxies actually primordial relics?
- Integral Field Spectroscopy of 23 Spiral Bulges
- A treatment procedure for GMOS/IFU data cubes: application to NGC 2835
- The continuous rise of bulges out of galactic disks
- ALMA [CI] observations toward the central region of a Seyfert galaxy NGC 613
- ALMA multiline observations toward the central region of NGC 613
- The nuclear region of NGC 613. I -- Multiwavelength analysis
- A SINFONI view of circum-nuclear star-forming rings in spiral galaxies