Unusual Broad Absorption Line Quasars from the Sloan Digital Sky Survey

Details Unusual Broad Absorption Line Quasars from the Sloan Digital Sky Survey Unusual Broad Absorption Line Quasars from the Sloan Digital Sky Survey

2002-03-15

arxiv.org/abs/astro-ph/0203252v1

Astrophys.J.Suppl.141:267,2002

Astronomy and Astrophysics

Astrophysics

ApJS in press. 50 pages, 27 bitmapped figures. Full resolution paper available at http://archive.stsci.edu/sdss/prepared_ds.ht

Scientific paper

10.1086/340546

The Sloan Digital Sky Survey has confirmed the existence of populations of broad absorption line (BAL) quasars with various unusual properties. We present and discuss twenty-three such objects and consider the implications of their wide range of properties for models of BAL outflows and quasars in general. We have discovered one BAL quasar with a record number of absorption lines. Two other similarly complex objects with many narrow troughs show broad MgII absorption extending longward of their systemic host galaxy redshifts. This can be explained as absorption of an extended continuum source by the rotation-dominated base of a disk wind. Five other objects have absorption which removes an unprecedented ~90% of all flux shortward of MgII. The absorption in one of them has varied across the ultraviolet with an amplitude and rate of change as great as ever seen. This same object may also show broad H-beta absorption. Numerous reddened BAL quasars have been found, including at least one reddened mini-BAL quasar with very strong FeII emission. The five reddest objects have continuum reddenings of E(B-V)~0.5, and in two of them we find strong evidence that the reddening curve is even steeper than that of the SMC. We have found at least one object with absorption from FeIII but not FeII. This may be due to a high column density of moderately high-ionization gas, but the FeIII level populations must also be affected by some sort of resonance. Finally, we have found two luminous, probably reddened high-redshift objects which may be BAL quasars whose troughs partially cover different regions of the continuum source as a function of velocity.

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