Biconical disk-wind models show that small acceleration length R_v plus high terminal velocity is required to produce detached blueshifted CIV absorption in synthetic spectra at intermediate inclinations.
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Wind Acceleration as a Driver of Detached Blueshifted Absorption in Quasar Disk Winds
Biconical disk-wind models show that small acceleration length R_v plus high terminal velocity is required to produce detached blueshifted CIV absorption in synthetic spectra at intermediate inclinations.