Measuring H-beta BLR Flows in NGC 5548

Details Measuring H-beta BLR Flows in NGC 5548 Measuring H-beta BLR Flows in NGC 5548

2007-07-17

arxiv.org/abs/0707.2606v1

Astronomy and Astrophysics

Astrophysics

2 pages, 2 figures; conference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M.

Scientific paper

Using archival International AGN Watch observations we find a correlation
between the asymmetry of the H-beta line and the system luminosity: the line
becomes bluer as the system gets brighter. We also find a differential lag
between the red and blue wings of the line: the blue wing lags the red by ~4
days, suggesting an inflow component of the BLR.

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