2003/10/22 by Chris J. Willott, Steve Rawlings, Willott, Chris J. +3
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0310653
To appear in the proceedings of "AGN Physics with the SDSS", eds. G. T. Richards and P. B. Hall (San Francisco: ASP) (2004), 4 pages including 1 figure, newpasp.sty
arxiv created 2003/10/22 · openalex publication_date 2003/10/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The results of a sub-millimeter survey of SDSS broad CIV absorption line\nquasars is discussed. It is found that the sub-millimeter flux distribution of\nBAL quasars is similar to that of non-BAL quasars. This is consistent with the\nidea that all quasars contain broad absorption line regions, but only a\nfraction of them are visible along our line-of-sight. The observations are\ninconsistent with BAL quasars being observed at a special evolutionary epoch\nco-inciding with a high star-formation rate and dust mass.\n