2017A&A...601A.143F


Query : 2017A&A...601A.143F

2017A&A...601A.143F - Astronomy and Astrophysics, volume 601A143-143 (2017/5-1)

AGN wind scaling relations and the co-evolution of black holes and galaxies.

FIORE F., FERUGLIO C., SHANKAR F., BISCHETTI M., BONGIORNO A., BRUSA M., CARNIANI S., CICONE C., DURAS F., LAMASTRA A., MAINIERI V., MARCONI A., MENCI N., MAIOLINO R., PICONCELLI E., VIETRI G. and ZAPPACOSTA L.

Abstract (from CDS):

Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as the main mechanism responsible for regulating star formation in active galactic nucleus (AGN) host galaxies. However, the relationships between AGN activity, radiation, winds, and star formation are complex and still far from being understood.
Aims. We study scaling relations between AGN properties, host galaxy properties, and AGN winds. We then evaluate the wind mean impact on the global star formation history, taking into account the short AGN duty cycle with respect to that of star formation.
Methods. We first collect AGN wind observations for 94 AGN with detected massive winds at sub-pc to kpc spatial scales. We then fold AGN wind scaling relations with AGN luminosity functions, to evaluate the average AGN wind mass-loading factor as a function of cosmic time.
Results. We find strong correlations between the AGN molecular and ionised wind mass outflow rates and the AGN bolometric luminosity. The power law scaling is steeper for ionised winds (slope 1.29±0.38) than for molecular winds (0.76±0.06), meaning that the two rates converge at high bolometric luminosities. The molecular gas depletion timescale and the molecular gas fraction of galaxies hosting powerful AGN driven winds are 3-10 times shorter and smaller than those of main sequence galaxies with similar star formation rate (SFR), stellar mass, and redshift. These findings suggest that, at high AGN bolometric luminosity, the reduced molecular gas fraction may be due to the destruction of molecules by the wind, leading to a larger fraction of gas in the atomic ionised phase. The AGN wind mass-loading factor η=MOF/SFR is systematically higher than that of starburst driven winds.
Conclusions. Our analysis shows that AGN winds are, on average, powerful enough to clean galaxies from their molecular gas only in massive systems at z≥2, i.e. a strong form of co-evolution between SMBHs and galaxies appears to break down for the least massive galaxies.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: active - galaxies: evolution - quasars: general - quasars: general

CDS comments: Table B.1 COS11363, COS43206, GS3-19791, GS3-28008, D3a-15504, I13120, Q1623 and U3-25105 not identified (incomplete format). MIRO 20581 is COSMOS 1647501.

Simbad objects: 89

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Number of rows : 89
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 [VV2006] J002830.5-281706 QSO 00 28 30.4642386648 -28 17 05.238885732     18.01     ~ 27 0
2 QSO B0109-353 QSO 01 11 43.6321128912 -35 03 00.587535660   16.6 16.9     ~ 79 0
3 LBQS 0109+0213 QSO 01 12 16.9871883144 +02 29 47.691927816   17 17.8     ~ 43 0
4 SDSS J014932.53-004803.7 Sy2 01 49 32.5267136928 -00 48 03.639150576   21.68 20.94     ~ 17 0
5 2XMM J021047.0-100152 Sy2 02 10 47.0026336728 -10 01 53.014352664   21.30 20.78     ~ 28 0
6 M 77 Sy2 02 42 40.7091669408 -00 00 47.859690204 9.70 9.61 8.87 10.1 9.9 ~ 4897 2
7 [CSB2004b] RG J030257.94+001016.3 AGN 03 02 57.94 +00 10 16.3         22.46 ~ 10 0
8 NGC 1266 Sy1 03 16 00.7739640240 -02 25 37.827013584   14   12.46   ~ 332 2
9 PKS J0318-2535 rG 03 18 12.091 -25 35 09.37   23.6 23.8     ~ 81 2
10 SDSS J031950.54-005850.6 Sy2 03 19 50.52255 -00 58 50.4099   22.17 21.48     ~ 18 0
11 SDSS J032144.11+001638.2 Sy2 03 21 44.11166 +00 16 38.1812   21.83 21.18     ~ 13 0
12 QSO B0329-385 QSO 03 31 06.3780612048 -38 24 04.653443772   17.63 16.92     ~ 85 1
13 NAME Chandra Deep Field-South reg 03 32 28.0 -27 48 30           ~ 2282 1
14 NGC 1433 Sy2 03 42 01.4847418992 -47 13 18.929092656   10.84 9.99 9.61 10.2 ~ 447 0
15 TXS 0406-244 QSO 04 08 51.463920 -24 18 16.40880     22.40     ~ 82 1
16 LB 1727 Sy1 04 26 00.7188165240 -57 12 01.769902992 13.68 14.58 14.37 14.8   ~ 307 0
17 4C 03.10 QSO 05 07 36.5037518903 +03 07 52.043712642     19.4     ~ 56 1
18 Z 395-23 Sy1 05 16 11.4092471904 -00 08 59.157166920   14.30 13.92     ~ 953 1
19 Z 235-30 Sy1 07 42 32.8210670808 +49 48 34.783809768   14.74 14.27     ~ 769 1
20 QSO J0745+4734 QSO 07 45 21.7878198936 +47 34 36.191801820   16.76 16.44     ~ 103 0
21 SDSS J075944.64+133945.7 Sy2 07 59 44.6390182704 +13 39 45.781131636   22.16 21.53     ~ 14 0
22 3C 191 QSO 08 04 47.9671662720 +10 15 23.746977252   18.65 18.40     ~ 295 2
23 NVSS J083053+191314 rG 08 30 53.507 +19 13 15.49           ~ 74 1
24 QSO J0831+5245 QSO 08 31 41.7108197808 +52 45 17.616994560   19.2   14.5 13.9 ~ 574 1
25 [VV2006] J083817.1+295526 QSO 08 38 17.0051826480 +29 55 26.531511276   18.84 18.42     ~ 52 0
26 SDSS J084130.77+204220.4 Sy2 08 41 30.7784805792 +20 42 20.428749684   22.13 21.46     ~ 16 0
27 LIRAS J084234.94+362503.2 Sy2 08 42 34.9476759744 +36 25 03.133827336   20.95 20.51     ~ 29 0
28 SDSS J085829.59+441734.6 Sy2 08 58 29.583816 +44 17 34.79460   19.72 19.39     ~ 18 0
29 IRAS 08572+3915 LIN 09 00 25.38288 +39 03 54.2988     16.66     ~ 450 1
30 QSO B0900+42 QSO 09 00 33.5091652824 +42 15 47.031009948   17.63 17.18     ~ 85 0
31 NAME SMM J09431+4700 AGN 09 43 03.96 +47 00 16.0       23.80   ~ 45 0
32 IRAS 09425+1751 Sy2 09 45 21.3401384376 +17 37 53.252237208   20.85 20.09     ~ 65 1
33 MCG-05-23-016 Sy2 09 47 40.1332188528 -30 56 55.960779696   14.10 13.69 12.44   ~ 611 0
34 LEDA 1463676 AGN 09 58 16.8923035632 +14 39 23.825430756           ~ 15 0
35 ACS-GC 20257695 rG 10 00 00.61 +02 15 31.1   25.596 25.580   24.826 ~ 42 0
36 2MASX J10001317+1242261 Sy2 10 00 13.1773284816 +12 42 26.446008420   19.03 18.34     ~ 28 0
37 ACS-GC 20000627 rG 10 02 11.27 +01 37 06.6 24.48 24.146 24.188   22.613 ~ 82 0
38 NVSS J100258+021018 rG 10 02 58.40537 +02 10 13.7733   22.278 22.318   21.45 ~ 33 0
39 SDSS J100308.84+020903.4 rG 10 03 08.865 +02 09 03.87   24.064 23.574     ~ 28 0
40 IRAS 10077+1427 Sy1 10 10 22.9567846176 +14 13 00.893737380   19.26 18.32     ~ 33 0
41 2MASS J10104334+0612013 Sy2 10 10 43.3642763928 +06 12 01.383491808   18.45 17.87     ~ 42 1
42 SDSS J103927.19+451215.2 Sy2 10 39 27.1982737728 +45 12 15.229723788   21.96 21.40     ~ 17 0
43 IRAS F10372+4801 Sy2 10 40 14.4383417952 +47 45 54.821962944   19.80 19.35     ~ 30 0
44 QSO J1044+3656 QSO 10 44 59.6100662544 +36 56 05.153586864   17.27 16.94     ~ 78 0
45 IRAS 10565+2448 LIN 10 59 18.12811 +24 32 34.7357   15.7       ~ 302 0
46 LEDA 3469502 Sy2 11 00 12.3868783440 +08 46 16.287755052   17.84 17.38     ~ 42 1
47 SDSS J110644.95+193930.6 QSO 11 06 44.9608950624 +19 39 30.623042844   19.87 19.47     ~ 21 0
48 NGC 3516 Sy1 11 06 47.4632200800 +72 34 07.298374656   13.12 12.40     ~ 1638 0
49 IRAS 11119+3257 Sy1 11 14 38.8902542640 +32 41 33.483258276   19.22 17.96     ~ 165 0
50 2MASS J11254636+1239225 Sy1 11 25 46.3629496704 +12 39 22.582294956           ~ 8 0
51 LEDA 3543738 Sy1 11 30 28.8694757040 +13 01 19.559875224           ~ 10 0
52 NGC 3783 Sy1 11 39 01.7096819040 -37 44 19.009642992   12.46 13.43 11.33 12.1 ~ 1765 1
53 PKS J1140-2628 rG 11 40 48.35884 -26 29 08.6316     22.00     ~ 325 1
54 SDSS J114816.64+525150.3 QSO 11 48 16.647 +52 51 50.31   25.73 25.04     ~ 487 0
55 QSO B1159+123 QSO 12 01 47.9118521640 +12 06 30.253926276   18.85 18.16     ~ 108 0
56 NGC 4051 Sy1 12 03 09.6101337312 +44 31 52.682601288   11.08 12.92 9.94   ~ 2270 1
57 NGC 4151 Sy1 12 10 32.5759813872 +39 24 21.063527532   12.18 11.48     ~ 3938 2
58 PB 3894 Sy1 12 14 17.6738687784 +14 03 13.182723144   14.46 14.19     ~ 873 0
59 QSO J1214+2803 QSO 12 14 42.3100795512 +28 03 29.156062824     17.30     ~ 48 0
60 NGC 4253 Sy1 12 18 26.5163572920 +29 48 46.531535472   14.34 13.57     ~ 1106 1
61 Mrk 205 BLL 12 21 44.0724099888 +75 18 38.241006228   15.64 15.24 14.7   ~ 492 0
62 NGC 4507 Sy2 12 35 36.6338976888 -39 54 33.710416272   12.95 13.54 11.70 12.4 ~ 532 1
63 QSO B1235+6219 QSO 12 37 16.0012375248 +62 03 23.351091948 19.9 20.55 20.19 19.9 19.5 ~ 64 0
64 Z 294-4 Sy1 12 56 14.2341182928 +56 52 25.238373852   14.68 13.84     ~ 2096 3
65 MCG-07-27-032 Sy1 13 06 26.1214861728 -40 24 52.595604396   13.58 13.42 12.01   ~ 269 0
66 2MASX J13150638-5509225 Sy2 13 15 06.33480 -55 09 22.7736   17.3       ~ 172 0
67 2MASS J13164290+1753326 Sy2 13 16 42.9031421040 +17 53 32.572818636   19.18 18.33     ~ 33 0
68 [VV2006] J132655.0-000531 QSO 13 26 54.9527826240 -00 05 30.134926968   21.22 20.81     ~ 37 0
69 2MASS J13395648+1425297 Sy1 13 39 56.4828086928 +14 25 29.626258980           ~ 6 0
70 IC 4329A Sy1 13 49 19.2601801224 -30 18 34.213815504   13.81 13.66 12.18 12.35 ~ 876 1
71 Z 336-28 Sy1 13 53 03.4348964112 +69 18 29.410910460   15.15 14.46     ~ 812 1
72 2MASS J13554566+1300509 Sy2 13 55 45.6680744544 +13 00 51.001910712           ~ 9 0
73 SDSS J135646.10+102609.0 Sy2 13 56 46.106 +10 26 09.09   18.90 18.11     ~ 95 0
74 NAME Teacup AGN Sy2 14 30 29.8820644560 +13 39 12.007458684   16.89 16.64     ~ 82 0
75 LEDA 89507 Sy2 14 40 59.0135478768 -37 04 31.938829896   17.72   16.48   ~ 131 1
76 Mrk 841 Sy1 15 04 01.1935384104 +10 26 15.780409692   14.50 14.27     ~ 701 0
77 Mrk 290 Sy1 15 35 52.4031021552 +57 54 09.515660508   15.55 15.27     ~ 575 0
78 2MASS J15493872+1245092 QSO 15 49 38.7147322320 +12 45 09.161026308   19.21 18.54 17.61   ~ 40 0
79 NAME SMM J163650.43+405734.5 Sy1 16 36 50.5 +40 57 34   23.3 23.30   21.83 ~ 91 0
80 NGC 6240 Sy2 16 52 58.9 +02 24 03   14.31 13.37     ~ 1734 2
81 LEDA 60189 LIN 17 23 21.96264 -00 17 00.8088   15.1       ~ 454 0
82 QSO B1725-142 QSO 17 28 19.7893499760 -14 15 55.854918288   14.69 14.03 13.7   ~ 362 0
83 Mrk 509 Sy1 20 44 09.7504483224 -10 43 24.727155528   13.35 13.12 10.7   ~ 1370 0
84 IC 5063 Bla 20 52 02.15 -57 04 06.7   12.92 13.60 11.30   ~ 710 1
85 IC 5066 G 20 57 03.0009659976 -73 08 49.754490324   15.14   14.19   ~ 11 0
86 NGC 7479 Sy2 23 04 56.6432243448 +12 19 22.357387020 11.74 11.60 10.85 10.47 9.66 ~ 783 2
87 IRAS 23060+0505 Sy1 23 08 33.9537309816 +05 21 29.751752412           ~ 160 0
88 LEDA 90429 SyG 23 39 01.26960 +36 21 08.5896   16.17       ~ 232 1
89 QSO J2359-1241 QSO 23 59 53.6307796320 -12 41 47.953525308     16.70     ~ 51 1

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