paper

THE POLARIZED SPECTRUM OF THE FE II-RICH BAL QSO, IRAS 07598+6508

arXiv:astro-ph/9505148 · doi:10.1086/309611

Abstract

We present IUE spectrophotometry and optical spectropolarimetry of the ultraluminous, extreme FeII-emitting QSO IRAS 07598+6508. We find broad absorption troughs from high- and low-ionization species, showing that this object is a member of the class of rare low-ionization BAL QSOs. Compared with non-BAL QSOs, the spectral energy distribution is reddened by E(B-V) sim 0.12, and the Halpha/Hbeta ratio even more reddened with E(B - V) sim 0.45. The broad emission lines are unpolarized. We see broad Na I lambda5892 absorption in the unpolarized continuum, but not in the polarized continuum (at the 5-6 sigma level). The polarized continuum rises smoothly towards shorter wavelengths with F_lambda propto lambda{-2}. We argue that a normal QSO continuum is polarized by scattering from a region within, or very near, the Broad Emission Line Region (BELR). Thus there are at least three distinct light paths to the observer: a dusty path from the BELR, a direct path traced by the unpolarized continuum, passing through dust and low-ionization gas (NaI), and another relatively unobscured path followed by scattered continuum. This provides direct evidence that a BAL region and dust only partially cover the central QSO. Ultraluminous AGNs, including IRAS 07598+6508, appear no more IR-luminous than non-IRAS-selected QSOs, and have normal L(IR)/L(opt) ratios when the optical luminosities are corrected for reddening. Reddening and BALs occur only along some sight lines and the parent population of BALQs are `normal' QSOs.

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