Matches in SemOpenAlex for { <https://semopenalex.org/work/W3105014233> ?p ?o ?g. }
- W3105014233 endingPage "A148" @default.
- W3105014233 startingPage "A148" @default.
- W3105014233 abstract "The aim of this paper is to test the basic model of negative AGN feedback. According to this model, once the central black hole accretes at the Eddington limit and reaches a certain critical mass, AGN driven outflows blow out gas, suppressing star formation in the host galaxy and self-regulating black hole growth. We consider a sample of 224 quasars selected from the SDSS at z<1 observed in the infrared band by Herschel. We evaluate the star formation rate in relation to several outflow signatures traced by the [OIII]4959,5007 and [OII]3726,3729 emission lines in about half of the sample with high quality spectra. Most of the quasars show asymmetric and broad wings in [OIII], which we interpret as outflow signatures. We separate the quasars in two groups, ``weakly'' and ``strongly'' outflowing, using three different criteria. When we compare the mean star formation rate in five redshift bins in the two groups, we find that the SFRs are comparable or slightly larger in the strongly outflowing quasars. We estimate the stellar mass from SED fitting and the quasars are distributed along the star formation main sequence, although with a large scatter. The scatter from this relation is uncorrelated with respect to the kinematic properties of the outflow. Moreover, for quasars dominated in the infrared by starburst or by AGN emission, we do not find any correlation between the star formation rate and the velocity of the outflow, a trend previously reported in the literature for pure starburst galaxies. We conclude that the basic AGN negative feedback scenario seems not to agree with our results. Although we use a large sample of quasars, we did not find any evidence that the star formation rate is suppressed in the presence of AGN driven outflows on large scale. A possibility is that feedback is effective over much longer timescales than those of single episodes of quasar activity." @default.
- W3105014233 created "2020-11-23" @default.
- W3105014233 creator A5002495372 @default.
- W3105014233 creator A5006901455 @default.
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- W3105014233 creator A5028319073 @default.
- W3105014233 creator A5034701878 @default.
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- W3105014233 creator A5061759484 @default.
- W3105014233 creator A5083337878 @default.
- W3105014233 creator A5084033977 @default.
- W3105014233 date "2016-01-01" @default.
- W3105014233 modified "2023-10-18" @default.
- W3105014233 title "Is there any evidence that ionized outflows quench star formation in type 1 quasars at<i>z</i>< 1?" @default.
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