2017A&A...603A..99P


C.D.S. - SIMBAD4 rel 1.7 - 2019.11.17CET09:45:55

2017A&A...603A..99P - Astronomy and Astrophysics, volume 603A, 99-99 (2017/7-1)

An X-ray/SDSS sample. I. Multi-phase outflow incidence and dependence on AGN luminosity.

PERNA M., LANZUISI G., BRUSA M., MIGNOLI M. and CRESCI G.

Abstract (from CDS):

Aims. The connection between the growth of super-massive black holes (SMBHs) and the evolution of their host galaxies is nowadays well established, although the underlying mechanisms explaining their mutual relations are still debated. Multi-phase fast, massive outflows have been postulated to play a crucial role in this process. The aim of this work is to constrain the nature and the fraction of outflowing gas in active galactic nuclei (AGNs) as well as the nuclear conditions possibly at the origin of such phenomena.
Methods. We present a large spectroscopic sample of X-ray detected SDSS AGNs at z<0.8 with a high signal-to-noise ratio in the [OIII]λ5007 line to unveil the faint wings of the emission profile associated with AGN-driven outflows. We used X-ray and optical flux ratio diagnostics to select the sample. We derived physical and kinematic characterization by re-analysing optical (and X-ray) spectra.
Results. We derive the incidence of ionized (∼40%) and atomic (<1%) outflows covering a wide range of AGN bolometric luminosity from 1042 to 1046erg/s. We also derive bolometric luminosities and X-ray bolometric corrections to test whether the presence of outflows is associated with an X-ray loudness, as suggested by our recent results obtained by studying high-z QSOs.
Conclusions. We study the relations between the outflow velocity inferred from [OIII] kinematic analysis and different AGN power tracers, such as black hole mass (MBH), [OIII], and X-ray luminosity. We show a well-defined positive trend between outflow velocity and LX, for the first time, over a range of 5 order of magnitudes. Overall, we find that in the QSO-luminosity regime and at MBH>108M the fraction of AGNs with outflows becomes >50%. Finally, we discuss our results about X-ray bolometric corrections and outflow incidence in cold and ionized phases in the context of an evolutionary sequence allowing two distinct stages for the feedback phase: first, an initial stage characterized by X-ray/optical obscured AGNs, in which the atomic gas is still present in the ISM and the outflow processes involve all the gas components and, second, a later stage associated with unobscured AGNs, in which the line of sight has been cleaned and the cold components have been heated or exhausted.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: active - quasars: emission lines - ISM: jets and outflows - ISM: jets and outflows

Simbad objects: 7

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Number of rows : 7

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 Mrk 1502 Sy1 00 53 34.9326560879 +12 41 35.927159668   14.41 14.03     ~ 1008 1
2 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 1894 0
3 2XMM J100211.2+013706 AGN 10 02 11.27 +01 37 06.6 24.48 24.146 24.188   22.613 ~ 43 0
4 2XMM J100308.8+020904 G 10 03 08.837 +02 09 03.41   24.064 23.574     ~ 24 0
5 Mrk 176 Sy2 11 32 40.2437529352 +52 57 01.304442422   15.50 14.61 13.52   ~ 225 2
6 Mrk 231 Sy1 12 56 14.2340989340 +56 52 25.238555193   14.68 13.84     ~ 1739 3
7 NAME IRAS F15163+4255 NW LIN 15 18 06.123 +42 44 44.59   15.0 15     ~ 175 1

    Equat.    Gal    SGal    Ecl

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2019.11.17-09:45:55

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