Polarization of Broad Absorption Line QSOs I. A Spectropolarimetric Atlas

Details Polarization of Broad Absorption Line QSOs I. A Spectropolarimetric Atlas Polarization of Broad Absorption Line QSOs I. A Spectropolarimetric Atlas

1999-05-24

arxiv.org/abs/astro-ph/9905299v1

Astrophys.J.Suppl. 125 (1999) 1-34

Astronomy and Astrophysics

Astrophysics

39 pages, 6 figures (20 .gif files), accepted for publication in The Astrophysical Journal Supplements

Scientific paper

10.1086/313272

We present a spectropolarimetric survey of 36 broad absorption line quasi-stellar objects (BAL QSOs). The continuum, absorption trough, and emission line polarization of BAL QSOs yield clues about their structure. We confirm that BAL QSOs are in general more highly polarized than non-BAL QSOs, consistent with a more equatorial viewing direction for the former than the latter. We have identified two new highly-polarized QSOs in our sample (1232+1325 and 1333+2840). The polarization rises weakly to the blue in most objects, perhaps due to scattering and absorption by dust particles. We find that a polarization increase in the BAL troughs is a general property of polarized BAL QSOs, indicating an excess of scattered light relative to direct light, and consistent with the unification of BAL QSOs and non-BAL QSOs. We have also discovered evidence of resonantly scattered photons in the red wing of the C IV broad emission lines of a few objects. In most cases, the broad emission lines have lower polarization and a different position angle than the continuum. The polarization characteristics of low-ionization BAL QSOs are similar to those of high-ionization BAL QSOs, suggesting a similar BAL wind geometry.

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