Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100858230> ?p ?o ?g. }
- W3100858230 endingPage "83" @default.
- W3100858230 startingPage "83" @default.
- W3100858230 abstract "Absorption spectroscopy of gravitationally lensed quasars (GLQs) enables study of spatial variations in the interstellar and/or circumgalactic medium of foreground galaxies. We report observations of 4 GLQs, each with two images separated by 0.8-3.0, that show strong absorbers at redshifts 0.4$<$$z_{abs}$$<$1.3 in their spectra, including some at the lens redshift with impact parameters 1.5-6.9 kpc. We measure H I Lyman lines along two sight lines each in five absorbers (10 sight lines in total) using HST STIS, and metal lines using Magellan Echellette or Sloan Digital Sky Survey. Our data have doubled the lens galaxy sample with measurements of H I column densities ($N_{rm H I}$) and metal abundances along multiple sight lines. Our data, combined with the literature, show no strong correlation between absolute values of differences in $N_{rm H I}$, $N_{rm Fe II}$, or [Fe/H] and the sight line separations at the absorber redshifts for separations of 0-8 kpc. The estimated abundance gradients show a tentative anti-correlation with abundances at galaxy centers. Some lens galaxies show inverted gradients, possibly suggesting central dilution by mergers or infall of metal-poor gas. [Fe/H] measurements and masses estimated from GLQ astrometry suggest the lens galaxies lie below the total mass-metallicity relation for early-type galaxies as well as measurements for quasar-galaxy pairs and gravitationally lensed galaxies at comparable redshifts. This difference may arise in part from the dust depletion of Fe. Higher resolution measurements of H and metals (especially undepleted elements) for more GLQ absorbers and accurate lens redshifts are needed to confirm these trends." @default.
- W3100858230 created "2020-11-23" @default.
- W3100858230 creator A5024676282 @default.
- W3100858230 creator A5042374450 @default.
- W3100858230 creator A5050899913 @default.
- W3100858230 creator A5060679701 @default.
- W3100858230 creator A5065148192 @default.
- W3100858230 creator A5071059947 @default.
- W3100858230 date "2019-11-22" @default.
- W3100858230 modified "2023-10-18" @default.
- W3100858230 title "Probing Structure in Cold Gas at <i>z</i> ≲ 1 with Gravitationally Lensed Quasar Sight Lines" @default.
- W3100858230 cites W1523639169 @default.
- W3100858230 cites W1539575775 @default.
- W3100858230 cites W1557591969 @default.
- W3100858230 cites W1573299053 @default.
- W3100858230 cites W1649074782 @default.
- W3100858230 cites W1799367687 @default.
- W3100858230 cites W1822844772 @default.
- W3100858230 cites W1829627820 @default.
- W3100858230 cites W1830177387 @default.
- W3100858230 cites W1835793325 @default.
- W3100858230 cites W1909741043 @default.
- W3100858230 cites W1969206417 @default.
- W3100858230 cites W1973412110 @default.
- W3100858230 cites W1975202273 @default.
- W3100858230 cites W1976888177 @default.
- W3100858230 cites W1979387507 @default.
- W3100858230 cites W1979829845 @default.
- W3100858230 cites W1986164846 @default.
- W3100858230 cites W1990370067 @default.
- W3100858230 cites W1992570077 @default.
- W3100858230 cites W1995333740 @default.
- W3100858230 cites W2007461622 @default.
- W3100858230 cites W2010356064 @default.
- W3100858230 cites W2011654732 @default.
- W3100858230 cites W2015110151 @default.
- W3100858230 cites W2016189541 @default.
- W3100858230 cites W2016847354 @default.
- W3100858230 cites W2021440252 @default.
- W3100858230 cites W2025800595 @default.
- W3100858230 cites W2030220646 @default.
- W3100858230 cites W2032949105 @default.
- W3100858230 cites W2035225065 @default.
- W3100858230 cites W2035684119 @default.
- W3100858230 cites W2036384042 @default.
- W3100858230 cites W2036930890 @default.
- W3100858230 cites W2038727728 @default.
- W3100858230 cites W2045563205 @default.
- W3100858230 cites W2045603377 @default.
- W3100858230 cites W2049166557 @default.
- W3100858230 cites W2050678027 @default.
- W3100858230 cites W2057439642 @default.
- W3100858230 cites W2057582805 @default.
- W3100858230 cites W2065560654 @default.
- W3100858230 cites W2067932525 @default.
- W3100858230 cites W2068895362 @default.
- W3100858230 cites W2069399805 @default.
- W3100858230 cites W2071186164 @default.
- W3100858230 cites W2077113345 @default.
- W3100858230 cites W2089728050 @default.
- W3100858230 cites W2096147217 @default.
- W3100858230 cites W2100054308 @default.
- W3100858230 cites W2116594012 @default.
- W3100858230 cites W2121547583 @default.
- W3100858230 cites W2123367369 @default.
- W3100858230 cites W2123924478 @default.
- W3100858230 cites W2124199755 @default.
- W3100858230 cites W2125835283 @default.
- W3100858230 cites W2132745107 @default.
- W3100858230 cites W2134203113 @default.
- W3100858230 cites W2153198268 @default.
- W3100858230 cites W2157603621 @default.
- W3100858230 cites W2157917411 @default.
- W3100858230 cites W2158091684 @default.
- W3100858230 cites W2159107767 @default.
- W3100858230 cites W2160269404 @default.
- W3100858230 cites W2165045150 @default.
- W3100858230 cites W2239733884 @default.
- W3100858230 cites W2259261862 @default.
- W3100858230 cites W2274830060 @default.
- W3100858230 cites W2289396866 @default.
- W3100858230 cites W2519558040 @default.
- W3100858230 cites W2520417698 @default.
- W3100858230 cites W2527653396 @default.
- W3100858230 cites W2604566923 @default.
- W3100858230 cites W2787073449 @default.
- W3100858230 cites W2790248196 @default.
- W3100858230 cites W2803501921 @default.
- W3100858230 cites W2895027382 @default.
- W3100858230 cites W2899497983 @default.
- W3100858230 cites W2916667240 @default.
- W3100858230 cites W2949884473 @default.
- W3100858230 cites W2952737353 @default.
- W3100858230 cites W2952953248 @default.
- W3100858230 cites W3098026053 @default.
- W3100858230 cites W3099298787 @default.
- W3100858230 cites W3099348560 @default.
- W3100858230 cites W3099896971 @default.