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- W2080920872 abstract "We assess the global properties of associated C IV λλ1548, 1550 absorption lines measured in the spectra of radio-loud quasars drawn from a near-complete, low-frequency-selected sample. The observations span rest-frame C IV in two redshift ranges, 0.7 < z < 1.0 and 1.5 < z < 3.0, which were targeted in the UV with the Hubble Space Telescope Space Telescope Imaging Spectrograph and in the optical with ground-based telescopes. First, we corroborate trends for C IV associated absorption to be found preferentially in steep-spectrum and lobe-dominated quasars, implying that the absorbing material tends to lie away from the radio-jet axis. Furthermore, we find a clear anticorrelation between C IV absorption strength and the projected linear size of steep-spectrum quasars, indicative of an evolutionary sequence. We also find that heavily absorbed quasars are systematically redder, implying that dust is mixed in with the C IV-absorbing gas. No redshift dependence was found in any of the trends considered. These new results show that radio sources are triggered in galaxies that are exceptionally rich in gas and dust, which then dissipates on a timescale comparable to but less than that of the radio source. This observational sequence, together with the lack of redshift dependence, points to a direct causal link between the event that triggered the radio source and the build-up of absorbing gas and dust, whose make-up is tantalizingly similar to the products of a postmerger starburst. Thus, these new results provide direct evidence for the clearing of absorbing material around quasars with time, as well as the probable association of starburst activity with the onset of the radio activity in active galactic nuclei." @default.
- W2080920872 created "2016-06-24" @default.
- W2080920872 creator A5005067544 @default.
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- W2080920872 date "2002-04-01" @default.
- W2080920872 modified "2023-09-25" @default.
- W2080920872 title "Associated Absorption in Radio Quasars. I. CivAbsorption and the Growth of Radio Sources" @default.
- W2080920872 cites W106178881 @default.
- W2080920872 cites W1497425588 @default.
- W2080920872 cites W176246254 @default.
- W2080920872 cites W1821182108 @default.
- W2080920872 cites W1851920400 @default.
- W2080920872 cites W1964218269 @default.
- W2080920872 cites W1965142997 @default.
- W2080920872 cites W1965568584 @default.
- W2080920872 cites W1966498099 @default.
- W2080920872 cites W1968043723 @default.
- W2080920872 cites W1970337765 @default.
- W2080920872 cites W1970604534 @default.
- W2080920872 cites W1972721631 @default.
- W2080920872 cites W1973938504 @default.
- W2080920872 cites W1979115990 @default.
- W2080920872 cites W1979898396 @default.
- W2080920872 cites W1986709885 @default.
- W2080920872 cites W1987276069 @default.
- W2080920872 cites W1987957756 @default.
- W2080920872 cites W1988354624 @default.
- W2080920872 cites W1991610844 @default.
- W2080920872 cites W1991812484 @default.
- W2080920872 cites W1993200911 @default.
- W2080920872 cites W1994657916 @default.
- W2080920872 cites W1994703407 @default.
- W2080920872 cites W1999166445 @default.
- W2080920872 cites W2005334789 @default.
- W2080920872 cites W2005972998 @default.
- W2080920872 cites W2007975728 @default.
- W2080920872 cites W2010090957 @default.
- W2080920872 cites W2010163489 @default.
- W2080920872 cites W2011383356 @default.
- W2080920872 cites W2011424601 @default.
- W2080920872 cites W2011543926 @default.
- W2080920872 cites W2014051101 @default.
- W2080920872 cites W2015260928 @default.
- W2080920872 cites W2016576409 @default.
- W2080920872 cites W2016856487 @default.
- W2080920872 cites W2020411139 @default.
- W2080920872 cites W2024696672 @default.
- W2080920872 cites W2026875764 @default.
- W2080920872 cites W2027058913 @default.
- W2080920872 cites W2027901034 @default.
- W2080920872 cites W2028425877 @default.
- W2080920872 cites W2031447477 @default.
- W2080920872 cites W2039521251 @default.
- W2080920872 cites W2043503871 @default.
- W2080920872 cites W2046988935 @default.
- W2080920872 cites W2047898352 @default.
- W2080920872 cites W2051967867 @default.
- W2080920872 cites W2054026519 @default.
- W2080920872 cites W2064826995 @default.
- W2080920872 cites W2066361364 @default.
- W2080920872 cites W2067045599 @default.
- W2080920872 cites W2067080837 @default.
- W2080920872 cites W2075669073 @default.
- W2080920872 cites W2080106878 @default.
- W2080920872 cites W2081240894 @default.
- W2080920872 cites W2081906145 @default.
- W2080920872 cites W2088853013 @default.
- W2080920872 cites W2088939813 @default.
- W2080920872 cites W2089436442 @default.
- W2080920872 cites W2090903589 @default.
- W2080920872 cites W2091282147 @default.
- W2080920872 cites W2092573091 @default.
- W2080920872 cites W2101150814 @default.
- W2080920872 cites W2110011261 @default.
- W2080920872 cites W2112615655 @default.
- W2080920872 cites W2114907309 @default.
- W2080920872 cites W2124219338 @default.
- W2080920872 cites W2131900813 @default.
- W2080920872 cites W2139502595 @default.
- W2080920872 cites W2145454176 @default.
- W2080920872 cites W2154722211 @default.
- W2080920872 cites W2154957141 @default.
- W2080920872 cites W2161532793 @default.
- W2080920872 cites W2161859140 @default.
- W2080920872 cites W2503443196 @default.
- W2080920872 cites W2726272604 @default.
- W2080920872 cites W2903101379 @default.
- W2080920872 cites W2950541171 @default.
- W2080920872 cites W3098205368 @default.
- W2080920872 cites W3098872520 @default.
- W2080920872 cites W3099047894 @default.
- W2080920872 cites W3099249414 @default.
- W2080920872 cites W3099352875 @default.