Fast outflows and star formation quenching in quasar host galaxies


Por: Carniani S., Marconi A., Maiolino R., Balmaverde B., Brusa M., Cano-Díaz M., Cicone C., Comastri A., Cresci G., Fiore F., Feruglio C., La Franca F., Mainieri V., Mannucci F., Nagao T., Netzer H., Piconcelli E., Risaliti G., Schneider R., Shemmer O.

Publicada: 1 jul 2016
Resumen:
Negative feedback from active galactic nuclei (AGN) is considered a key mechanism in shaping galaxy evolution. Fast, extended outflows are frequently detected in the AGN host galaxies at all redshifts and luminosities, both in ionised and molecular gas. However, these outflows are only potentially able to quench star formation, and we are still lacking decisive evidence of negative feedback in action. Here we present observations obtained with the Spectrograph for INtegral Field Observations in the Near Infrared (SINFONI) H- and K-band integral-field of two quasars at z similar to 2.4 that are characterised by fast, extended outflows detected through the [OIII]lambda 5007 line. The high signal-to-noise ratio of our observations allows us to identify faint narrow (FWHM < 500 km s(-1)) and spatially extended components in [OIII]lambda 5007 and H alpha emission associated with star formation in the host galaxy. This star formation powered emission is spatially anti-correlated with the fast outflows. The ionised outflows therefore appear to be able to suppress star formation in the region where the outflow is expanding. However, the detection of narrow spatially extended H alpha emission indicates star formation rates of at least similar to 50-90 M-circle dot yr(-1), suggesting either that AGN feedback does not affect the whole galaxy or that many feedback episodes are required before star formation is completely quenched. On the other hand, the narrow H alpha emission extending along the edges of the outflow cone may also lead also to a positive feedback interpretation. Our results highlight the possible double role of galaxy-wide outflows in host galaxy evolution.

Filiaciones:
Carniani S.:
 Univ Florence, Dipartimento Fis & Astron, Via G Sansone 1, I-50019 Florence, Italy

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

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

 Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

 Dipartimento di Fisica e Astronomia, Università di Firenze, via G. Sansone 1, Sesto Fiorentino (Firenze), 50019, Italy

 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze, 50125, Italy

 Cavendish Laboratory, University of Cambridge, 19 J. J. Thomson Ave., Cambridge, CB3 0HE, United Kingdom

 Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom

Marconi A.:
 Univ Florence, Dipartimento Fis & Astron, Via G Sansone 1, I-50019 Florence, Italy

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

 Dipartimento di Fisica e Astronomia, Università di Firenze, via G. Sansone 1, Sesto Fiorentino (Firenze), 50019, Italy

 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze, 50125, Italy

Maiolino R.:
 Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England

 Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

 Cavendish Laboratory, University of Cambridge, 19 J. J. Thomson Ave., Cambridge, CB3 0HE, United Kingdom

 Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom

Balmaverde B.:
 Univ Florence, Dipartimento Fis & Astron, Via G Sansone 1, I-50019 Florence, Italy

 Dipartimento di Fisica e Astronomia, Università di Firenze, via G. Sansone 1, Sesto Fiorentino (Firenze), 50019, Italy

Brusa M.:
 Univ Bologna, Dipartimento Fis & Astron, Viale Berti Pichat 6-2, I-40127 Bologna, Italy

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

 Dipartimento di Fisica e Astronomia, Università di Bologna, viale Berti Pichat 6/2, Bologna, 40127, Italy

 INAF, Osservatorio Astronomico di Bologna, via Ranzani 1, Bologna, 40127, Italy

Cano-Díaz M.:
 Univ Nacl Autonoma Mexico, Inst Astron, Apartado Postal 70-264, Mexico City 04510, DF, Mexico

 Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, México D.F., 04510, Mexico

Cicone C.:
 ETH, Dept Phys, Inst Astron, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland

 Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, Zurich, 8093, Switzerland

Comastri A.:
 INAF Osservatorio Astron Bologna, Via Ranzani 1, I-40127 Bologna, Italy

 INAF, Osservatorio Astronomico di Bologna, via Ranzani 1, Bologna, 40127, Italy

Cresci G.:
 INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze, 50125, Italy

Fiore F.:
 INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy

 INAF, Osservatorio Astronomico di Roma, via Frascati 33, Monteporzio Catone, 00040, Italy

Feruglio C.:
 INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy

 Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy

 IRAM Inst RadioAstron Millimetr, 300 Rue Piscine, F-38406 St Martin Dheres, France

 INAF, Osservatorio Astronomico di Roma, via Frascati 33, Monteporzio Catone, 00040, Italy

 Scuola Normale Superiore, Piazza dei Cavalieri 7, Pisa, 56126, Italy

 IRAM-Institut de RadioAstronomie Millimétrique, 300 rue de la Piscine, Saint-Martin d Hères, 38406, France

La Franca F.:
 Univ Rome Tre, Dipartimento Matemat & Fis, Via Vasca Navale 84, I-00146 Rome, Italy

 Dipartimento di Matematica e Fisica, Università Roma Tre, via della Vasca Navale 84, Roma, 00146, Italy

Mainieri V.:
 European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

 European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei München, 85748, Germany

Mannucci F.:
 INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze, 50125, Italy

Nagao T.:
 Ehime Univ, Res Ctr Space & Cosm Evolut, Bunkyo Cho 2-5, Matsuyama, Ehime 7908577, Japan

 Research Center for Space and Cosmic Evolution, Ehime University, Bunkyo-cho 2-5, Matsuyama, Ehime, 790-8577, Japan

Netzer H.:
 Tel Aviv Univ, Sackler Fac Exact Sci, Sch Phys & Astron, IL-69978 Tel Aviv, Israel

 School of Physics and Astronomy, Sackler Faculty of Exact Sciences, Tel-Aviv University, Tel-Aviv, 69978, Israel

Piconcelli E.:
 INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy

 INAF, Osservatorio Astronomico di Roma, via Frascati 33, Monteporzio Catone, 00040, Italy

Risaliti G.:
 INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze, 50125, Italy

Schneider R.:
 INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy

 INAF, Osservatorio Astronomico di Roma, via Frascati 33, Monteporzio Catone, 00040, Italy

Shemmer O.:
 Univ North Texas, Dept Phys, Denton, TX 76203 USA

 Department of Physics, University of North Texas, Denton, TX 76203, United States
ISSN: 00046361
Editorial
EDP SCIENCES S A, 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE, Francia
Tipo de documento: Article
Volumen: 591 Número:
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WOS Id: 000379141300037