Matches in SemOpenAlex for { <https://semopenalex.org/work/W4384636142> ?p ?o ?g. }
- W4384636142 endingPage "3145" @default.
- W4384636142 startingPage "3130" @default.
- W4384636142 abstract "We present the first systematic study of the molecular gas and star formation efficiency in a sample of ten narrow-line Seyfert 1 galaxies selected to have X-ray Ultra Fast Outflows and, therefore, to potentially show AGN feedback effects. CO observations were obtained with the IRAM 30m telescope in six galaxies and from the literature for four galaxies. We derived the stellar mass, star formation rate, AGN and FIR dust luminosities by fitting the multi-band spectral energy distributions with the CIGALE code. Most of the galaxies in our sample lie above the main sequence (MS) and the molecular depletion time is one to two orders of magnitude shorter than the one typically measured in local star-forming galaxies. Moreover, we found a promising correlation between the star formation efficiency and the Eddington ratio, as well as a tentative correlation with the AGN luminosity. The role played by the AGN activity in the regulation of star formation within the host galaxies of our sample remains uncertain (little or no effect? positive feedback?). Nevertheless, we can conclude that quenching by the AGN activity is minor and that star formation will likely stop in a short time due to gas exhaustion by the current starburst episode." @default.
- W4384636142 created "2023-07-19" @default.
- W4384636142 creator A5014966782 @default.
- W4384636142 creator A5016187719 @default.
- W4384636142 creator A5021988166 @default.
- W4384636142 creator A5031028129 @default.
- W4384636142 creator A5035322080 @default.
- W4384636142 creator A5039128270 @default.
- W4384636142 creator A5047541804 @default.
- W4384636142 creator A5056282733 @default.
- W4384636142 creator A5060807711 @default.
- W4384636142 creator A5077274038 @default.
- W4384636142 date "2023-07-12" @default.
- W4384636142 modified "2023-10-15" @default.
- W4384636142 title "Star formation efficiency and AGN feedback in narrow-line Seyfert 1 galaxies with fast X-ray nuclear winds" @default.
- W4384636142 cites W139336091 @default.
- W4384636142 cites W1660326066 @default.
- W4384636142 cites W1660434781 @default.
- W4384636142 cites W1842880767 @default.
- W4384636142 cites W1857068670 @default.
- W4384636142 cites W1925665838 @default.
- W4384636142 cites W1966671782 @default.
- W4384636142 cites W1974353009 @default.
- W4384636142 cites W1974646076 @default.
- W4384636142 cites W1975524662 @default.
- W4384636142 cites W1979369985 @default.
- W4384636142 cites W1985952407 @default.
- W4384636142 cites W1989095107 @default.
- W4384636142 cites W1989372921 @default.
- W4384636142 cites W1994671833 @default.
- W4384636142 cites W1996537612 @default.
- W4384636142 cites W2003472160 @default.
- W4384636142 cites W2005501750 @default.
- W4384636142 cites W2011297915 @default.
- W4384636142 cites W2012612847 @default.
- W4384636142 cites W2016829294 @default.
- W4384636142 cites W2019398523 @default.
- W4384636142 cites W2020814246 @default.
- W4384636142 cites W2025621984 @default.
- W4384636142 cites W2035318083 @default.
- W4384636142 cites W2037298232 @default.
- W4384636142 cites W2043989216 @default.
- W4384636142 cites W2048414711 @default.
- W4384636142 cites W2052937506 @default.
- W4384636142 cites W2059634633 @default.
- W4384636142 cites W2070354775 @default.
- W4384636142 cites W2072327312 @default.
- W4384636142 cites W2077888380 @default.
- W4384636142 cites W2079831217 @default.
- W4384636142 cites W2082322112 @default.
- W4384636142 cites W2092504858 @default.
- W4384636142 cites W2096517145 @default.
- W4384636142 cites W2102600871 @default.
- W4384636142 cites W2103914245 @default.
- W4384636142 cites W2113005372 @default.
- W4384636142 cites W2116466430 @default.
- W4384636142 cites W2121404382 @default.
- W4384636142 cites W2123267088 @default.
- W4384636142 cites W2129760210 @default.
- W4384636142 cites W2135536375 @default.
- W4384636142 cites W2136565048 @default.
- W4384636142 cites W2137064512 @default.
- W4384636142 cites W2142220522 @default.
- W4384636142 cites W2143213816 @default.
- W4384636142 cites W2149063305 @default.
- W4384636142 cites W2150995848 @default.
- W4384636142 cites W2151062050 @default.
- W4384636142 cites W2153037851 @default.
- W4384636142 cites W2155421027 @default.
- W4384636142 cites W2157917411 @default.
- W4384636142 cites W2589052511 @default.
- W4384636142 cites W2589201834 @default.
- W4384636142 cites W2593258774 @default.
- W4384636142 cites W2600114070 @default.
- W4384636142 cites W2604243687 @default.
- W4384636142 cites W2612511799 @default.
- W4384636142 cites W2761208967 @default.
- W4384636142 cites W2788794673 @default.
- W4384636142 cites W2804337859 @default.
- W4384636142 cites W2883576199 @default.
- W4384636142 cites W2885255958 @default.
- W4384636142 cites W2898179605 @default.
- W4384636142 cites W2899552690 @default.
- W4384636142 cites W2918006881 @default.
- W4384636142 cites W2949496523 @default.
- W4384636142 cites W2950786244 @default.
- W4384636142 cites W2952725678 @default.
- W4384636142 cites W2963030616 @default.
- W4384636142 cites W2991323708 @default.
- W4384636142 cites W2992593518 @default.
- W4384636142 cites W3002888012 @default.
- W4384636142 cites W3012251357 @default.
- W4384636142 cites W3027862860 @default.
- W4384636142 cites W3084299552 @default.
- W4384636142 cites W3088871662 @default.
- W4384636142 cites W3089275552 @default.
- W4384636142 cites W3092066260 @default.
- W4384636142 cites W3095875787 @default.