The Intrinsic Absorber in Qso 2359–1241: Keck and Hst Observations

We present detailed analyses of the absorption spectrum seen in QSO 2359– 1241 (NVSS J235953−124148). Keck HIRES data reveal absorption from twenty transitions arising from: He i, Mg i, Mg ii, Ca ii, and Fe ii. HST data show broad absorption lines (BALs) from Al iii λ1857, C iv λ1549, Si iv λ1397, and Nv λ1240. Absorption from excited Fe ii states constrains the temperature of the absorber to 2000 < ∼ T < ∼ 10, 000 K and puts a lower limit of 10 5 cm on the electron number density. Saturation diagnostics show that the real column densities of He i and Fe ii can be determined, allowing to derive meaningful constraints on the ionization equilibrium and abundances in the flow. The ionization parameter is constrained by the iron, helium and magnesium data to −3.0 < ∼ log(U) < ∼ −2.5 and the observed column densities can be reproduced without assuming departure from solar abundances. From comparison of the He i and Fe ii absorption features we infer that the outflow seen in QSO 2359–1241 is not shielded by a hydrogen ionization front and therefore that the existence of low-ionization species in the outflow (e.g., Mg ii, Al iii, Fe ii) does not necessitate the existence of such a front. We find that the velocity width of the absorption systematically increases as a function of ionization and to a lesser extent with abundance. Complementary analyses of the radio and polarization properties of the object are discussed in a companion paper (Brotherton et al. 2000). Subject headings: quasars: absorption lines Physics Department, University of California, Davis, CA 95616 I: [email protected] 2 Kitt Peak National Observatory, 950 North Cherry Avenue, P. O. Box 26732, Tuscon, AZ 85726 IGPP LLNL, L-413, P.O. Box 808, Livermore, CA 94550 Space Telescope Science Institute, Baltimore, MD 21218