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Narrow associated QSO absorbers: clustering, outflows and the
line-of-sight proximity effect
Narrow associated QSO absorbers: clustering, outflows and the
line-of-sight proximity effect
2008-02-27
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arxiv.org/abs/0802.4100v1
Mon.Not.Roy.Astron.Soc.388:227-241,2008
Astronomy and Astrophysics
Astrophysics
16 pages, 20 figures, submitted to MNRAS
Scientific paper
10.1111/j.1365-2966.2008.13375.x
Using data from the Sloan Digital Sky Survey data release 3 (SDSS DR3) we investigate how narrow (<700km/s) CIV and MgII quasar absorption line systems are distributed around quasars. The CIV absorbers lie in the redshift range 1.6 < z < 4 and the MgII absorbers in the range 0.440% of CIV absorbers within 3,000km/s of the QSO are not a result of large-scale clustering but rather are directly associated with the quasar itself; (iii) that this intrinsic absorber population extends to outflow velocities of order 12,000km/s; (iv) that this outflow component is present in both radio-loud and radio-quiet quasars; and (v) that a small high-velocity outflow component is observed in the MgII population, but any further intrinsic absorber component is undetectable in our clustering analysis. We also find an indication that absorption systems within 3,000km/s are more abundant for radio-loud than for radio-quiet quasars. This suggests either that radio-loud objects live in more massive halos, or that their radio activity generates an additional low-velocity outflow, or both.
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