Work

Keplerian Motion of Broad-Line Region Gas as Evidence for Supermassive Black Holes in Active Galactic Nuclei

Year: 1999
Type: article
Abstract: Emission-line variability data on NGC 5548 argue strongly for the existence of a mass of order 7 × 10 7 M ☉ within the inner few light-days of the nucleus in the Seyfert 1 galaxy NGC 5548. The time-delayed response of the emission lines to continuum variations is used to infer the size of the line-emitting region, and these determinations are combined with measurements of the Doppler widths of the variable line components to estimate a virial mass. The data for several different emission lines spanning an order of magnitude in distance from the central source show the expected V ∝ r -1/2 correlation and are consistent with a single value for the mass.
Authors: Bradley M. Peterson, Amri Wandel
Language: English
Open Access status: bronze
OpenAlex ID: W2049399829
FWCI: 10.58
Cites: 23
Cited by: 361
Related to: 10