We present a dynamical model in which the broad absorption lines seen in some quasar
spectra form in a smooth nonspherical wind from an accretion disk. On the inner edge of this …

… & Chiang The 1981; Murray 1996). lines in cataclysmic variables come in two forms,
double… Murray & Chiang argue that one di†erence between the two cases is that highluminosity …

… The Civ absorption can be used to predict the column density and the intrinsic ox (Murray
& Chiang 1995). The fact that all these objects are lobe-dominated or steep-spectrum sources …

… However, the radiative-transfer e†ects we describe (Murray 1995). here will apply to any …
analytical –ts to photoionization calculations that we report on elsewhere (Murray & Chiang …

… More recently, Murray and Chiang" showed explicitly how radiative transfer effects in the
base of the wind ensure that the profiles produced in AGN disks are singlepeaked. Here we use …

We present a model for radiation-driven winds from accretion disks in active galactic nuclei.
In particular, we discuss how X-ray shielding allows resonance-line radiation pressure to …

… radiative transfer effects in the outflow (Murray & Chiang 1996). In this contribution we
argue that the blueshifted absorption seen in quasars and AGNs is … We refer the reader to�…

We present a dynamical model in which the broad absorption lines (BALs) seen in some
quasar spectra form in a smooth non-spherical wind from an accretion disk. On the inner edge …

… & Chiang (1997a) have shown how the broad emission lines (BELs) seen in all …
phenomena can be explained by this model (Murray & Chiang 1997b; Chiang & Murray�…

… (Murray & Chiang 1996). The emission comes from the region where the gas is accelerated
away from the surface of the disk. This gas is rotating at the local Keplerian velocity, with a …