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- W3105291241 abstract "We analyze the results of long-term observations of the broad-line region (BLR) in the Seyfert 1 galaxy NGC 5548 and provide a critical comparison with the predictions of a hydromagnetically driven outflow model of Emmering, Blandford, & Shlosman. We use this model to generate a time series of C IV line profiles that have responded to a time-varying continuum. Our modifications to the model include cloud emission anisotropy, cloud obscuration, a CLOUDY-generated emissivity function, and a narrow-line component which is added to the BLR component to generate the total line profiles. The model is driven with continuum input based on the monitoring campaigns of NGC 5548 reported in Clavel et al. and Korista et al., and the line strengths, profiles, and lags are compared with the observations." @default.
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- W3105291241 date "1997-04-10" @default.
- W3105291241 modified "2023-09-23" @default.
- W3105291241 title "Dynamics of Broad Emission‐Line Region in NGC 5548: Hydromagnetic Wind Model versus Observations" @default.
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- W3105291241 doi "https://doi.org/10.1086/303867" @default.
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