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• W3166192767 endingPage "902" @default.
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• W3166192767 abstract "(Abridged) We present a systematic investigation of physical conditions and elemental abundances in four optically thick Lyman-limit systems (LLSs) at $z=0.36-0.6$ discovered within the Cosmic Ultraviolet Baryon Survey (CUBS). CUBS LLSs exhibit multi-component kinematic structure and a complex mix of multiphase gas, with associated metal transitions from multiple ionization states that span several hundred km/s in line-of-sight velocity. Specifically, higher column density components (log N(HI)>16) in all four absorbers comprise dynamically cool gas with $langle T rangle =(2pm1) times10^4,$K and modest non-thermal broadening of $5pm3,$ km/s. The high quality of the QSO absorption spectra allows us to infer the physical conditions of the gas, using a detailed ionization modeling that takes into account the resolved component structures of HI and metal transitions. The range of inferred gas densities indicates that these absorbers consist of spatially compact clouds with a median line-of-sight thickness of $160^{+140}_{-50}$ pc. While obtaining robust metallicity constraints for the low-density, highly ionized phase remains challenging due to the uncertain N(HI), we demonstrate that the cool-phase gas in LLSs has a median metallicity of $mathrm{[alpha/H]_{1/2}}=-0.7^{+0.1}_{-0.2}$, with a 16-84 percentile range of $mathrm{[alpha/H]}=(-1.3,-0.1)$. Furthermore, the wide range of inferred elemental abundance ratios ($mathrm{[C/alpha]}$, $mathrm{[N/alpha]}$, and $mathrm{[Fe/alpha]}$) indicate a diversity of chemical enrichment histories. Combining the absorption data with deep galaxy survey data characterizing the galaxy environment of these absorbers, we discuss the physical connection between star-forming regions in galaxies and diffuse gas associated with optically thick absorption systems in the $z<1$ circumgalactic medium." @default.
• W3166192767 created "2021-06-22" @default.
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• W3166192767 date "2021-06-22" @default.
• W3166192767 modified "2023-10-18" @default.
• W3166192767 title "The Cosmic Ultraviolet Baryon Survey (CUBS) – III. Physical properties and elemental abundances of Lyman-limit systems at <i>z</i> &lt; 1" @default.
• W3166192767 cites W1573037074 @default.
• W3166192767 cites W1634574618 @default.
• W3166192767 cites W1768240921 @default.
• W3166192767 cites W1914270569 @default.
• W3166192767 cites W1932831857 @default.
• W3166192767 cites W1965767581 @default.
• W3166192767 cites W1966022526 @default.
• W3166192767 cites W1968438730 @default.
• W3166192767 cites W1971083632 @default.
• W3166192767 cites W1975202273 @default.
• W3166192767 cites W2004958755 @default.
• W3166192767 cites W2006160097 @default.
• W3166192767 cites W2006716028 @default.
• W3166192767 cites W2016656456 @default.
• W3166192767 cites W2028466334 @default.
• W3166192767 cites W2035684119 @default.
• W3166192767 cites W2039013407 @default.
• W3166192767 cites W2042417147 @default.
• W3166192767 cites W2046939760 @default.
• W3166192767 cites W2049430551 @default.
• W3166192767 cites W2050287260 @default.
• W3166192767 cites W2051770437 @default.
• W3166192767 cites W2057448325 @default.
• W3166192767 cites W2067857092 @default.
• W3166192767 cites W2068895362 @default.
• W3166192767 cites W2074646278 @default.
• W3166192767 cites W2076396726 @default.
• W3166192767 cites W2080386153 @default.
• W3166192767 cites W2119037421 @default.
• W3166192767 cites W2119135771 @default.
• W3166192767 cites W2125473068 @default.
• W3166192767 cites W2128071918 @default.
• W3166192767 cites W2152671803 @default.
• W3166192767 cites W2157594202 @default.
• W3166192767 cites W2161137739 @default.
• W3166192767 cites W2161196919 @default.
• W3166192767 cites W2162064299 @default.
• W3166192767 cites W2164096156 @default.
• W3166192767 cites W2165045150 @default.
• W3166192767 cites W2167597203 @default.
• W3166192767 cites W2258614408 @default.
• W3166192767 cites W2289396866 @default.
• W3166192767 cites W2331439334 @default.
• W3166192767 cites W2366704018 @default.
• W3166192767 cites W2410852485 @default.
• W3166192767 cites W2512213311 @default.
• W3166192767 cites W2531220143 @default.
• W3166192767 cites W2539770846 @default.
• W3166192767 cites W2558282339 @default.
• W3166192767 cites W2565714260 @default.
• W3166192767 cites W2568336518 @default.
• W3166192767 cites W2597238720 @default.
• W3166192767 cites W2613587629 @default.
• W3166192767 cites W2616996827 @default.
• W3166192767 cites W2625910788 @default.
• W3166192767 cites W2762265283 @default.
• W3166192767 cites W2771069682 @default.
• W3166192767 cites W2785832652 @default.
• W3166192767 cites W2887297741 @default.
• W3166192767 cites W2890363482 @default.
• W3166192767 cites W2899497983 @default.
• W3166192767 cites W2923999595 @default.
• W3166192767 cites W2949001442 @default.
• W3166192767 cites W2962876139 @default.
• W3166192767 cites W2963661167 @default.
• W3166192767 cites W3003988923 @default.
• W3166192767 cites W3021886534 @default.
• W3166192767 cites W3093729840 @default.
• W3166192767 cites W3098223162 @default.
• W3166192767 cites W3098325361 @default.
• W3166192767 cites W3098466678 @default.
• W3166192767 cites W3098703286 @default.

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