Polarization in lines - a new method for measuring black hole masses in active galaxies
arXiv:1501.07730 · doi:10.1088/2041-8205/800/2/L35
Abstract
Measuring of the masses of galactic supermassive black holes (SMBHs) is an important task, since they correlate with the host galaxy properties and play an important role in evolution of galaxies. Here we present a new method for measuring of SMBH masses using the polarization of the broad lines emitted from active galactic nuclei (AGNs). We performed spectropolarometric observations of 9 AGNs and find that this method gives measured masses which are in a good agreement with reverberation measurements. An advantage of this method is that it can be used to measure the masses of SMBHs in a consistent way at different cosmological epochs.
arXiv commentApJL accepted
References in corpus (13)
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
- The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
- Reverberation Mapping Measurements of Black Hole Masses in Six Local Seyfert Galaxies
- Reverberation Measurements of the Inner Radius of the Dust Torus in 17 Seyfert Galaxies
- Reverberation Mapping Results for Five Seyfert 1 Galaxies
- What broad emission lines tell us about how active galactic nuclei work
- Convective Overstability in radially stratified accretion disks under thermal relaxation
- The innermost dusty structure in active galactic nuclei as probed by the Keck interferometer
- NGC 5548 in a Low-Luminosity State: Implications for the Broad-Line Region
- Equatorial scattering and the structure of the broad-line region in Seyfert nuclei: evidence for a rotating disc
- Variability in Spectropolarimetric properties of Sy 1.5 galaxy Mrk 6
- Analysis of a Fragmenting Sunspot using Hinode Observations
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- Determination of the Physical Parameters of AGNs in Seyfert 1 Galaxies LEDA 3095839 and VII Zw 244 Based on Spectropolarimetric Observations
- Probing AGN with spectropolarimetry: accretion disk and SMBH parameters
- Comparison between the influence of outflows and supermassive binary black holes in active galactic nuclei on the polarization angle profiles
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