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

被引：447

作者：

Fiore, F. ^{[1
]}

Feruglio, C. ^{[2
]}

Shankar, F. ^{[3
]}

Bischetti, M. ^{[1
]}

Bongiorno, A. ^{[1
]}

Brusa, M. ^{[4
,5
]}

Carniani, S. ^{[6
,7
]}

Cicone, C. ^{[8
,9
]}

Duras, F. ^{[1
]}

Lamastra, A. ^{[1
]}

Mainieri, V. ^{[10
]}

Marconi, A. ^{[6
,11
]}

Menci, N. ^{[1
]}

Maiolino, R. ^{[7
]}

Piconcelli, E. ^{[1
]}

Vietri, G. ^{[1
]}

Zappacosta, L. ^{[1
]}

机构：

[1] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[2] INAF Osservatorio Astron Trieste, Via G Tiepolo 11, I-34124 Trieste, Italy

[3] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England

[4] Univ Bologna, Dipartimento Fis & Astron, Alma Mater Studiorum, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

[5] INAF Osservatorio Astron Bologna, Via Ranzani 1, I-40127 Bologna, Italy

[6] Univ Firenze, Dipartimento Fis & Astron, Via G Sansone 1, I-50019 Florence, Italy

[7] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England

[8] INAF Osservatorio Astron Brera, Via Brera 28, I-20121 Milan, Italy

[9] ETH, Dept Phys, Inst Astron, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland

[10] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[11] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

来源：

ASTRONOMY & ASTROPHYSICS | 2017年 / 601卷

基金：

欧盟地平线“2020”; 瑞士国家科学基金会;

关键词：

galaxies: active; galaxies: evolution; quasars: general; ACTIVE GALACTIC NUCLEUS; X-RAY LUMINOSITY; ULTRALUMINOUS INFRARED GALAXIES; LARGE TELESCOPE OBSERVATIONS; FAST MOLECULAR OUTFLOWS; STAR-FORMING GALAXIES; RADIO-QUIET QUASARS; ULTRA-FAST OUTFLOWS; HOST GALAXIES; HELLAS2XMM SURVEY;

D O I：

10.1051/0004-6361/201629478

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 eta = M-OF /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 less than or similar to 2, i.e. a strong form of co-evolution between SMBHs and galaxies appears to break down for the least massive galaxies.

引用

页数：21

共 189 条

[1] High resolution observations of HCN and HCO+ J=3-2 in the disk and outflow of Mrk 231 Detection of vibrationally excited HCN in the warped nucleus [J].

Aalto, S. ;

Garcia-Burillo, S. ;

Muller, S. ;

Winters, J. M. ;

Gonzalez-Alfonso, E. ;

van der Werf, P. ;

Henkel, C. ;

Costagliola, F. ;

Neri, R. .

ASTRONOMY & ASTROPHYSICS, 2015, 574

[2] Detection of HCN, HCO+, and HNC in the Mrk 231 molecular outflow Dense molecular gas in the AGN wind [J].

Aalto, S. ;

Garcia-Burillo, S. ;

Muller, S. ;

Winters, J. M. ;

van der Werf, P. ;

Henkel, C. ;

Costagliola, F. ;

Neri, R. .

ASTRONOMY & ASTROPHYSICS, 2012, 537

[3] The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z∼5 [J].

Aird, J. ;

Coil, A. L. ;

Georgakakis, A. ;

Nandra, K. ;

Barro, G. ;

Perez-Gonzalez, P. G. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 451 (02) :1892-1927

[4] The evolution of the hard X-ray luminosity function of AGN [J].

Aird, J. ;

Nandra, K. ;

Laird, E. S. ;

Georgakakis, A. ;

Ashby, M. L. N. ;

Barmby, P. ;

Coil, A. L. ;

Huang, J. -S. ;

Koekemoer, A. M. ;

Steidel, C. C. ;

Willmer, C. N. A. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 401 (04) :2531-2551

[5] DISCOVERY OF AN ACTIVE GALACTIC NUCLEUS DRIVEN MOLECULAR OUTFLOW IN THE LOCAL EARLY-TYPE GALAXY NGC 1266 [J].

Alatalo, K. ;

Blitz, L. ;

Young, L. M. ;

Davis, T. A. ;

Bureau, M. ;

Lopez, L. A. ;

Cappellari, M. ;

Scott, N. ;

Shapiro, K. L. ;

Crocker, A. F. ;

Martin, S. ;

Bois, M. ;

Bournaud, F. ;

Davies, R. L. ;

de Zeeuw, P. T. ;

Duc, P. -A. ;

Emsellem, E. ;

Falcon-Barroso, J. ;

Khochfar, S. ;

Krajnovic, D. ;

Kuntschner, H. ;

Lablanche, P. -Y. ;

McDermid, R. M. ;

Morganti, R. ;

Naab, T. ;

Oosterloo, T. ;

Sarzi, M. ;

Serra, P. ;

Weijmans, A. .

ASTROPHYSICAL JOURNAL, 2011, 735 (02)

[6] NGC 1266 AS A LOCAL CANDIDATE FOR RAPID CESSATION OF STAR FORMATION [J].

Alatalo, Katherine ;

Nyland, Kristina ;

Graves, Genevieve ;

Deustua, Susana ;

Griffin, Kristen Shapiro ;

Duc, Pierre-Alain ;

Cappellari, Michele ;

McDermid, Richard M. ;

Davis, Timothy A. ;

Crocker, Alison F. ;

Young, Lisa M. ;

Chang, Philip ;

Scott, Nicholas ;

Cales, Sabrina L. ;

Bayet, Estelle ;

Blitz, Leo ;

Bois, Maxime ;

Bournaud, Frederic ;

Bureau, Martin ;

Davies, Roger L. ;

de Zeeuw, P. T. ;

Emsellem, Eric ;

Khochfar, Sadegh ;

Krajnovic, Davor ;

Kuntschner, Harald ;

Morganti, Raffaella ;

Naab, Thorsten ;

Oosterloo, Tom ;

Sarzi, Marc ;

Serra, Paolo ;

Weijmans, Anne-Marie .

ASTROPHYSICAL JOURNAL, 2014, 780 (02)

[7] Searching for evidence of energetic feedback in distant galaxies: a galaxy wide outflow in a z ≈ 2 ultraluminous infrared galaxy [J].

Alexander, D. M. ;

Swinbank, A. M. ;

Smail, Ian ;

McDermid, R. ;

Nesvadba, N. P. H. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 402 (04) :2211-2220

[8] The Chandra Deep Field North Survey. X. X-ray emission from very red objects [J].

Alexander, DM ;

Vignali, C ;

Bauer, FE ;

Brandt, WN ;

Hornschemeier, AE ;

Garmire, GP ;

Schneider, DP .

ASTRONOMICAL JOURNAL, 2002, 123 (03) :1149-1162

[9] Hubble Space Telescope images of a sample of 20 nearby luminous quasars [J].

Bahcall, JN ;

Kirhakos, S ;

Saxe, DH ;

Schneider, DP .

ASTROPHYSICAL JOURNAL, 1997, 479 (02) :642-&

[10] DISTANCE TO MULTIPLE KINEMATIC COMPONENTS OF QUASAR OUTFLOWS: VERY LARGE TELESCOPE OBSERVATIONS OF QSO 2359-1241 AND SDSS J0318-0600 [J].

Bautista, Manuel A. ;

Dunn, Jay P. ;

Arav, Nahum ;

Korista, Kirk T. ;

Moe, Maxwell ;

Benn, Chris .

ASTROPHYSICAL JOURNAL, 2010, 713 (01) :25-31

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