Matches in SemOpenAlex for { <https://semopenalex.org/work/W2897319605> ?p ?o ?g. }
- W2897319605 endingPage "3932" @default.
- W2897319605 startingPage "3915" @default.
- W2897319605 abstract "Large scale outflows of different gas phases are ubiquitous in the host galaxies of active galactic nuclei (AGN). Despite their many differences, they share a common property - they all contain dust. The dust is carried with the outflow, heated by the AGN, and emits at infrared wavelengths. This paper shows that the infrared emission of this dust can be used to detect AGN outflows and derive their properties. We use a sample of about 4000 type II AGN and compare the infrared properties of systems that show spectroscopic signature of ionized gas outflows to systems that do not. We detect an additional mid-infrared emission component in galaxies with spectroscopically discovered winds, and attribute it to the dust in the outflow. This new component offers novel constraints on the outflow properties, such as its mean location and covering factor. We measure the location of the outflow for roughly 1700 systems, with the distribution showing a prominent peak around 500 pc, a tail that extends to large distances (10 kpc), and no objects with a location smaller than 50 pc. The covering factor of the wind shows a wide distribution which is centered around 0.1, with 24% (8%) of the winds showing covering factors larger than 0.2 (0.5). The dust emission is not sensitive to various systematics affecting optically-selected outflows, and can be used to estimate the mass outflow rate in thousands of galaxies with only 1D spectra." @default.
- W2897319605 created "2018-10-26" @default.
- W2897319605 creator A5053592523 @default.
- W2897319605 creator A5086132801 @default.
- W2897319605 date "2018-11-01" @default.
- W2897319605 modified "2023-09-27" @default.
- W2897319605 title "Discovering AGN-driven winds through their infrared emission – I. General method and wind location" @default.
- W2897319605 cites W1558119406 @default.
- W2897319605 cites W1683186775 @default.
- W2897319605 cites W1966193056 @default.
- W2897319605 cites W1967876247 @default.
- W2897319605 cites W1967920531 @default.
- W2897319605 cites W1973808059 @default.
- W2897319605 cites W1988249910 @default.
- W2897319605 cites W1989095107 @default.
- W2897319605 cites W1998878332 @default.
- W2897319605 cites W2002044265 @default.
- W2897319605 cites W2004503258 @default.
- W2897319605 cites W2016904340 @default.
- W2897319605 cites W2026156043 @default.
- W2897319605 cites W2027297109 @default.
- W2897319605 cites W2045798320 @default.
- W2897319605 cites W2052937506 @default.
- W2897319605 cites W2056945538 @default.
- W2897319605 cites W2061939373 @default.
- W2897319605 cites W2067857092 @default.
- W2897319605 cites W2069477144 @default.
- W2897319605 cites W2070458043 @default.
- W2897319605 cites W2078959782 @default.
- W2897319605 cites W2080927107 @default.
- W2897319605 cites W2082732658 @default.
- W2897319605 cites W2084264738 @default.
- W2897319605 cites W2114138701 @default.
- W2897319605 cites W2115652448 @default.
- W2897319605 cites W2117307008 @default.
- W2897319605 cites W2124199755 @default.
- W2897319605 cites W2127657174 @default.
- W2897319605 cites W2135894620 @default.
- W2897319605 cites W2142220522 @default.
- W2897319605 cites W2147847259 @default.
- W2897319605 cites W2150364524 @default.
- W2897319605 cites W2166365370 @default.
- W2897319605 cites W2169224160 @default.
- W2897319605 cites W2200610228 @default.
- W2897319605 cites W2249695201 @default.
- W2897319605 cites W2255006479 @default.
- W2897319605 cites W2285880218 @default.
- W2897319605 cites W2291265024 @default.
- W2897319605 cites W2309252738 @default.
- W2897319605 cites W2339708160 @default.
- W2897319605 cites W2559430844 @default.
- W2897319605 cites W2581997630 @default.
- W2897319605 cites W2589052511 @default.
- W2897319605 cites W2613782670 @default.
- W2897319605 cites W2618457610 @default.
- W2897319605 cites W2626242135 @default.
- W2897319605 cites W2789436540 @default.
- W2897319605 cites W2791766821 @default.
- W2897319605 cites W2796698519 @default.
- W2897319605 cites W2798556224 @default.
- W2897319605 cites W3098140412 @default.
- W2897319605 cites W3098450776 @default.
- W2897319605 cites W3099105840 @default.
- W2897319605 cites W3099149995 @default.
- W2897319605 cites W3099592869 @default.
- W2897319605 cites W3099644107 @default.
- W2897319605 cites W3100679294 @default.
- W2897319605 cites W3100981399 @default.
- W2897319605 cites W3101070241 @default.
- W2897319605 cites W3101377002 @default.
- W2897319605 cites W3101518584 @default.
- W2897319605 cites W3101694449 @default.
- W2897319605 cites W3101755663 @default.
- W2897319605 cites W3103271302 @default.
- W2897319605 cites W3103317920 @default.
- W2897319605 cites W3103428888 @default.
- W2897319605 cites W3103655493 @default.
- W2897319605 cites W3104330986 @default.
- W2897319605 cites W3105111674 @default.
- W2897319605 cites W3105161400 @default.
- W2897319605 cites W3105356976 @default.
- W2897319605 cites W3105480099 @default.
- W2897319605 cites W3105913662 @default.
- W2897319605 cites W3106274047 @default.
- W2897319605 cites W3106383930 @default.
- W2897319605 cites W3124194601 @default.
- W2897319605 cites W3124221423 @default.
- W2897319605 cites W3124241678 @default.
- W2897319605 cites W3125306729 @default.
- W2897319605 cites W4295973521 @default.
- W2897319605 doi "https://doi.org/10.1093/mnras/sty2935" @default.
- W2897319605 hasPublicationYear "2018" @default.
- W2897319605 type Work @default.
- W2897319605 sameAs 2897319605 @default.
- W2897319605 citedByCount "26" @default.
- W2897319605 countsByYear W28973196052019 @default.
- W2897319605 countsByYear W28973196052020 @default.
- W2897319605 countsByYear W28973196052021 @default.