Matches in SemOpenAlex for { <https://semopenalex.org/work/W4387409028> ?p ?o ?g. }
- W4387409028 endingPage "54" @default.
- W4387409028 startingPage "54" @default.
- W4387409028 abstract "Abstract Our knowledge of the circumgalactic medium (CGM) is mostly based on quasar absorption line measurements. These have uncovered a multiphase medium that is likely highly turbulent, but constraints of this turbulence are limited to measurements of the nonthermal width of absorption line components ( b turb ) and the line-of-sight velocity dispersion between components ( σ LOS ). Here we analyze a suite of CGM simulations to determine how well these indirect measures are related to the underlying CGM. Our simulations track the nonequilibrium evolution of all commonly observed ions and consist of two main types: small-scale simulations of regions of homogenous CGM turbulence and global simulations of inhomogenous turbulence throughout a galactic halo. From each simulation, we generate mock spectra of Si ii , Si iv , C iv , and O vi , which allow us to directly compare b turb and σ LOS to the true line-of-sight turbulence ( σ 1D ). In the small-scale simulations, b turb is only weakly correlated with σ 1D , likely because it measures random motions within individual warm CGM clouds, which do not sample the overall random motions. Meanwhile, σ LOS and σ 1D are strongly correlated with σ 1D ≈ σ LOS + 10 km s −1 in the densest regions we simulated, although the strength of this correlation depended weakly on the gas phase being probed. Our large-scale simulations also indicate that b turb and σ 1D are largely uncorrelated and that σ 1D ≈ σ LOS + 10 km s −1 on average, although it varies along individual sight lines. Moreover, the σ LOS distributions from our global simulations are similar to recent observations, suggesting that this quantity may provide useful constraints on circumgalactic turbulence regardless of the axis probed." @default.
- W4387409028 created "2023-10-07" @default.
- W4387409028 creator A5017169700 @default.
- W4387409028 creator A5028683533 @default.
- W4387409028 creator A5073236929 @default.
- W4387409028 date "2023-10-01" @default.
- W4387409028 modified "2023-10-08" @default.
- W4387409028 title "Constraining Circumgalactic Turbulence with QSO Absorption Line Measurements" @default.
- W4387409028 cites W1516675624 @default.
- W4387409028 cites W1589061681 @default.
- W4387409028 cites W1688406301 @default.
- W4387409028 cites W1882938068 @default.
- W4387409028 cites W1978574709 @default.
- W4387409028 cites W1986303447 @default.
- W4387409028 cites W2001085255 @default.
- W4387409028 cites W2004310296 @default.
- W4387409028 cites W2006160097 @default.
- W4387409028 cites W2011301426 @default.
- W4387409028 cites W2012886609 @default.
- W4387409028 cites W2017957151 @default.
- W4387409028 cites W2046275384 @default.
- W4387409028 cites W2058210847 @default.
- W4387409028 cites W2064888972 @default.
- W4387409028 cites W2067468675 @default.
- W4387409028 cites W2068262275 @default.
- W4387409028 cites W2083871083 @default.
- W4387409028 cites W2095325710 @default.
- W4387409028 cites W2099314289 @default.
- W4387409028 cites W2105153534 @default.
- W4387409028 cites W2118385522 @default.
- W4387409028 cites W2118534222 @default.
- W4387409028 cites W2124417513 @default.
- W4387409028 cites W2134717193 @default.
- W4387409028 cites W2142763738 @default.
- W4387409028 cites W2152118050 @default.
- W4387409028 cites W2157482862 @default.
- W4387409028 cites W2243603935 @default.
- W4387409028 cites W2462347146 @default.
- W4387409028 cites W2465705021 @default.
- W4387409028 cites W2530043748 @default.
- W4387409028 cites W2590752565 @default.
- W4387409028 cites W2594781706 @default.
- W4387409028 cites W2763851688 @default.
- W4387409028 cites W2798325923 @default.
- W4387409028 cites W2885525563 @default.
- W4387409028 cites W2895970607 @default.
- W4387409028 cites W2903538469 @default.
- W4387409028 cites W2954930523 @default.
- W4387409028 cites W2962995700 @default.
- W4387409028 cites W2966527379 @default.
- W4387409028 cites W3021886534 @default.
- W4387409028 cites W3036770410 @default.
- W4387409028 cites W3037641373 @default.
- W4387409028 cites W3098466678 @default.
- W4387409028 cites W3099383736 @default.
- W4387409028 cites W3099420115 @default.
- W4387409028 cites W3099464599 @default.
- W4387409028 cites W3099878876 @default.
- W4387409028 cites W3100161494 @default.
- W4387409028 cites W3100351477 @default.
- W4387409028 cites W3101366992 @default.
- W4387409028 cites W3101876501 @default.
- W4387409028 cites W3102165226 @default.
- W4387409028 cites W3102266975 @default.
- W4387409028 cites W3102743132 @default.
- W4387409028 cites W3102766224 @default.
- W4387409028 cites W3103050756 @default.
- W4387409028 cites W3103138619 @default.
- W4387409028 cites W3103609701 @default.
- W4387409028 cites W3103688182 @default.
- W4387409028 cites W3103782454 @default.
- W4387409028 cites W3103877238 @default.
- W4387409028 cites W3104305918 @default.
- W4387409028 cites W3104790555 @default.
- W4387409028 cites W3105959567 @default.
- W4387409028 cites W3106192069 @default.
- W4387409028 cites W3106325365 @default.
- W4387409028 cites W3166192767 @default.
- W4387409028 cites W4214923176 @default.
- W4387409028 cites W4292136310 @default.
- W4387409028 cites W4297183616 @default.
- W4387409028 cites W4376124492 @default.
- W4387409028 cites W4385706489 @default.
- W4387409028 cites W887389825 @default.
- W4387409028 doi "https://doi.org/10.3847/1538-4357/acf4fc" @default.
- W4387409028 hasPublicationYear "2023" @default.
- W4387409028 type Work @default.
- W4387409028 citedByCount "0" @default.
- W4387409028 crossrefType "journal-article" @default.
- W4387409028 hasAuthorship W4387409028A5017169700 @default.
- W4387409028 hasAuthorship W4387409028A5028683533 @default.
- W4387409028 hasAuthorship W4387409028A5073236929 @default.
- W4387409028 hasBestOaLocation W43874090281 @default.
- W4387409028 hasConcept C120665830 @default.
- W4387409028 hasConcept C121332964 @default.
- W4387409028 hasConcept C125287762 @default.
- W4387409028 hasConcept C1276947 @default.
- W4387409028 hasConcept C135041427 @default.