MODELING THE DOUBLE-TROUGH STRUCTURE OBSERVED IN BROAD ABSORPTION-LINE QSOS USING RADIATIVE ACCELERATION

We present a model explaining the double trough, separated by DELTAupsilon approximately 5900 km s-1, observed in the C IV lambda1549 broad absorption line (BAL) in a number of BALQSOs. The model is based on radiative acceleration of the BAL outflow, and the troughs result from modulations in the radiative force. Specifically, where the strong flux from the Lyalpha lambda1215 broad emission line is redshifted to the frequency of the N v lambda1240 resonance line, in the rest frame of the accelerating N v ions, the acceleration increases and the absorption is reduced. At higher velocities the Lyalpha emission is redshifted out of the resonance and the N v ions experience a. declining flux which causes the second absorption trough. A strongly nonlinear relationship between changes in the flux and the optical depth in the lines is shown to amplify the expected effect. This model produces double troughs for which the shallowest absorption between the two troughs occurs at upsilon congruent-to 5900 km s-1. Indeed, we find that a substantial number of the observed objects show this feature. A prediction of the model is that all BALQSOs that show a double-trough signature will be found to have an intrinsic sharp drop in their spectra shortward of approximately 1200 angstrom.