Dynamical Mass of Type 2 Seyfert Nuclei
arXiv:astro-ph/9803044 · doi:10.1086/305646
Abstract
We have derived the masses of central objects () of nine type 2 Seyfert nuclei using the observational properties of the hidden broad H emission. We obtain the average dynamical mass, log where is the optical depth for electron scattering. If , this average mass is almost comparable with those of type 1 Seyfert nuclei. However, if , as is usually considered, the average mass of type 2 Seyfert nuclei may be more massive than that of type 1s. We discuss implications for issues concerning both the current unified model of Seyfert nuclei and physical conditions of the electron scattering regions.
21 pages, 2 figures; accepted for Astrophysical Journal
References in corpus (1)
Cited by in corpus (9)
- The Flaring H2O Megamaser and Compact Radio Source in Mrk 348
- Chandra High Energy Grating Observations of the Fe Ka Line Core in Type 2 Seyfert Galaxies: A Comparison with Type 1 Nuclei
- X-ray emission from Seyfert 2 galaxies with optical polarized broad lines
- Sensitive VLBI Continuum and H I Absorption Observations of NGC 7674: First Scientific Observations with the Combined Array VLBA, VLA & Arecibo
- A New Black Hole Mass Estimate for Obscured Active Galactic Nuclei
- Was 49b: An Overmassive AGN in a Merging Dwarf Galaxy?
- A variability study of the Seyfert 2 galaxy NGC 6300 with XMM-Newton
- The Electron Scattering Region in Seyfert Nuclei
- Monitoring RXTE Observations of Markarian 348: the origin of the column density variations