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19 April 2024
 
  » arxiv » astro-ph/9810287

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A Statistical Study of Rest-frame Optical Emission Properties in Luminous Quasars at 2.0 < z < 2.5
D. H. McIntosh ; M. J. Rieke ; H.-W. Rix ; C. B. Foltz ; R. J. Weymann ;
Date 19 Oct 1998
Journal Astrophys.J. 514 (1999) 40
Subject astro-ph
AffiliationSteward Obs./Univ. of Ariz.), C. B. Foltz (Multiple Mirror Telescope Obs.), and R. J. Weymann (Carnegie Institute
AbstractWe have obtained H-band spectra of 32 luminous quasars at 2.095%) differences between the rest-frame optical emission line properties of the BALQSO and nonBALQSO subsamples. This result is consistent with the view that all RQQs have broad-absorption-line clouds with a small (~10-20%) covering factor and that differences between the two types are merely a function of viewing angle and covering factor. (4) We report a previously unknown luminosity and/or redshift dependence of the narrow-line-region velocity width over the range 0
Source arXiv, astro-ph/9810287
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