Abstract
A large, high-quality spectral data base of well-selected, moderate-redshift radio-loud and radio-quiet quasars is used to characterize the incidence of narrow associated CIV lambda 1549 absorption, and how this may depend on some quasar properties, including radio-type. Preliminary results of this study are presented.
Original language | English |
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Journal | Astronomical Society of the Pacific. Conference Proceedings |
Volume | 255 |
Pages (from-to) | 143 |
Number of pages | 1 |
ISSN | 1050-3390 |
Publication status | Published - 21 Sept 2002 |
Keywords
- astro-ph