A morphological comparison between the central region in AGN and normal galaxies using HST data
arXiv:astro-ph/0203376 · doi:10.1051/0004-6361:20020429
Abstract
We study the morphology of the central region of a sample of Active Galactic Nuclei (AGN) and a ``control'' sample of normal galaxies using archival observations of the WFPC2 instrument onboard the Hubble Space Telescope (HST). We use the ellipse fitting technique in order to get a good description of the inner ``smooth'' light distribution of the galaxy. We then divide the observed galaxy image by the artificial image from the fitted ellipses in order to detect morphological signatures in the central region around the nucleus of the galaxy. We perform quantitative comparisons of different subgroups of our sample of galaxies (according to the Hubble type and the nuclear activity of the galaxies) by calculating the average amplitude of the structures that are revealed with the ellipse fitting technique. Our main conclusions are as follows: 1) All AGNs show significant structure in their inner 100 pc and 1 kpc regions whose amplitude is similar in all of them, independent of the Hubble type of the host galaxy. 2) When considering early-type galaxies, non-AGN galaxies show no structure at all, contrary to what we find for AGN. 3) When considering late-type galaxies, both AGN and non-AGN galaxies show significant structure in their central region. Our results are consistent with the hypothesis that all early-type galaxies host a supermassive black hole, but only those that have enough material in the central regions to fuel it show an active nucleus. The situation is more complicated in late-type galaxies. Either not all of them host a central black hole, or, in some of them, the material inside the innermost 100 pc region is not transported to the scales of the central engine for some reason, or the large amount of gas and dust hides the active nucleus from our sight.
Accepted for publication in A&A. A gziped ps file with high resolution figures is available at http://armonia.physics.uoc.gr/~xilouris/publications/pub.html
References in corpus (4)
- Using Hubble Space Telescope Imaging of Nuclear Dust Morphology to Rule Out Bars Fueling Seyfert Nuclei
- Hubble Space Telescope Observations of the CfA Seyfert 2s: The Fueling of Active Galactic Nuclei
- The Frequency of Active and Quiescent Galaxies with Companions: Implications for the Feeding of the Nucleus
- Near-infrared photometry of isolated spirals with and without an AGN. I: The Data
Cited by in corpus (11)
- Determining Inclinations of Active Galactic Nuclei Via Their Narrow-Line Region Kinematics - I. Observational Results
- A Strong Correlation between Circumnuclear Dust and Black Hole Accretion in Early-Type Galaxies
- The blue host galaxy of the red GRB 000418
- Determining Inclinations of Active Galactic Nuclei Via Their Narrow-Line Region Kinematics - II. Correlation With Observed Properties
- Spectral and morphological properties of quasar hosts in SPH simulations of AGN feeding by mergers
- Optical multiband surface photometry of a sample of Seyfert galaxies. I. Large-scale morphology and local environment analysis of matched Seyfert and inactive galaxy samples
- Infrared-red Cores in Nearby Elliptical Galaxies
- Circumnuclear Structures in Megamaser Host Galaxies
- The X-ray variability and the near-IR to X-ray spectral energy distribution of four low luminosity Seyfert 1 galaxies
- Galaxy Interaction and Starburst-Seyfert Connection
- Demonstration of KVN phase referencing capability