Matches in SemOpenAlex for { <https://semopenalex.org/work/W3022331010> ?p ?o ?g. }
- W3022331010 endingPage "320" @default.
- W3022331010 startingPage "305" @default.
- W3022331010 abstract "We analyze VLT/X-shooter data for 7 quasars, where we study the relationships between their broad absorption line (BAL) and emission line outflows. We find: 1) the luminosity of the [OIII] $lambda$5007 emission profile decreases with increasing electron number density (n$_e$) derived from the BAL outflow in the same quasar, 2) the measured velocity widths from the [OIII] emission features and CIV absorption troughs in the same object are similar, and 3) the mean radial velocity derived from the BAL outflow is moderately larger than the one from the [OIII] emission outflow. These findings can be explained by the physical interpretation that the [OIII] and BAL outflow are different manifestations of the same wind. When we have outflows with smaller distances to the central source, their n$_e$ is higher. Therefore, the [OIII] emission is collisionally de-excited and the [OIII] luminosity is then suppressed. Comparisons to previous studies show that the objects in our sample exhibit broad [OIII] emission features similar to the ones in extremely red quasars (ERQs). This might imply that BAL quasars and ERQs have the same geometry of outflows or are at a similar evolutionary stage. We found that the physical parameters derived from the BAL outflows can explain the amount of observed [OIII] luminosity, which strengthens our claim of both BAL and [OIII] outflows are from the same wind. These estimates can be tested with upcoming James Webb Space Telescope observations." @default.
- W3022331010 created "2020-05-13" @default.
- W3022331010 creator A5032520367 @default.
- W3022331010 creator A5054924454 @default.
- W3022331010 creator A5062742011 @default.
- W3022331010 creator A5072812038 @default.
- W3022331010 creator A5080747598 @default.
- W3022331010 date "2020-05-04" @default.
- W3022331010 modified "2023-10-16" @default.
- W3022331010 title "Evidence that emission and absorption outflows in quasars are related" @default.
- W3022331010 cites W1516675624 @default.
- W3022331010 cites W1587885137 @default.
- W3022331010 cites W1632840073 @default.
- W3022331010 cites W1701063863 @default.
- W3022331010 cites W1763069159 @default.
- W3022331010 cites W1798382770 @default.
- W3022331010 cites W1958545965 @default.
- W3022331010 cites W1972336358 @default.
- W3022331010 cites W1977604962 @default.
- W3022331010 cites W1989762217 @default.
- W3022331010 cites W1990988314 @default.
- W3022331010 cites W1992469153 @default.
- W3022331010 cites W2001872772 @default.
- W3022331010 cites W2005501750 @default.
- W3022331010 cites W2014028747 @default.
- W3022331010 cites W2015229210 @default.
- W3022331010 cites W2016904340 @default.
- W3022331010 cites W2019839650 @default.
- W3022331010 cites W2027058913 @default.
- W3022331010 cites W2027297109 @default.
- W3022331010 cites W2027901034 @default.
- W3022331010 cites W2032531787 @default.
- W3022331010 cites W2036319176 @default.
- W3022331010 cites W2039153199 @default.
- W3022331010 cites W2041216883 @default.
- W3022331010 cites W2042710206 @default.
- W3022331010 cites W2044610256 @default.
- W3022331010 cites W2046722348 @default.
- W3022331010 cites W2053229150 @default.
- W3022331010 cites W2066744800 @default.
- W3022331010 cites W2067468675 @default.
- W3022331010 cites W2070458043 @default.
- W3022331010 cites W2073838033 @default.
- W3022331010 cites W2078900625 @default.
- W3022331010 cites W2079040992 @default.
- W3022331010 cites W2085689319 @default.
- W3022331010 cites W2101300883 @default.
- W3022331010 cites W2101380525 @default.
- W3022331010 cites W2117307008 @default.
- W3022331010 cites W2127657174 @default.
- W3022331010 cites W2135443317 @default.
- W3022331010 cites W2137901692 @default.
- W3022331010 cites W2144925347 @default.
- W3022331010 cites W2147925360 @default.
- W3022331010 cites W2150840048 @default.
- W3022331010 cites W2162351375 @default.
- W3022331010 cites W2245716257 @default.
- W3022331010 cites W2270888872 @default.
- W3022331010 cites W2291265024 @default.
- W3022331010 cites W2316324992 @default.
- W3022331010 cites W2525578541 @default.
- W3022331010 cites W2569002896 @default.
- W3022331010 cites W2585972288 @default.
- W3022331010 cites W2595429534 @default.
- W3022331010 cites W2738760779 @default.
- W3022331010 cites W2773785565 @default.
- W3022331010 cites W2797537565 @default.
- W3022331010 cites W2800172336 @default.
- W3022331010 cites W2803763743 @default.
- W3022331010 cites W2887909489 @default.
- W3022331010 cites W2891245903 @default.
- W3022331010 cites W2891277906 @default.
- W3022331010 cites W2897615793 @default.
- W3022331010 cites W2909220465 @default.
- W3022331010 cites W2913673111 @default.
- W3022331010 cites W2945575599 @default.
- W3022331010 cites W2947898882 @default.
- W3022331010 cites W2948101605 @default.
- W3022331010 cites W2949319977 @default.
- W3022331010 cites W2949496523 @default.
- W3022331010 cites W2963145381 @default.
- W3022331010 cites W2980772444 @default.
- W3022331010 cites W3022668787 @default.
- W3022331010 cites W3098517356 @default.
- W3022331010 cites W3098801911 @default.
- W3022331010 cites W3099295528 @default.
- W3022331010 cites W3100521758 @default.
- W3022331010 cites W3100526457 @default.
- W3022331010 cites W3100530628 @default.
- W3022331010 cites W3100556126 @default.
- W3022331010 cites W3100564466 @default.
- W3022331010 cites W3100825082 @default.
- W3022331010 cites W3101836047 @default.
- W3022331010 cites W3102283863 @default.
- W3022331010 cites W3103142496 @default.
- W3022331010 cites W3103234226 @default.
- W3022331010 cites W3103398559 @default.
- W3022331010 cites W3104542987 @default.