AGN wind scaling relations and the co-evolution of black holes and galaxies
F. FioreINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyC. FeruglioINAF–Osservatorio Astronomico di Trieste, via G. Tiepolo 11, 34124 Trieste, ItalyFrancesco ShankarDepartment of Physics and Astronomy, University of Southampton, Highfield, SO17 1BJ, UKM. BischettiINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyA. BongiornoINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyM. BrusaDipartimento di Fisica e Astronomia, Alma Mater Studiorum – Universitá di Bologna, viale Berti Pichat 6/2, 40127 Bologna, ItalyStefano CarnianiCavendish Laboratory, University of Cambridge, 19 J. J. Thomson Ave., Cambridge CB3 0HE, UKC. CiconeETH, Institute for Astronomy, Department of Physics, Wolfgang-Pauli-Strasse 278093 Zurich, SwitzerlandF. DurasINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyA. LamastraINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyV. MainieriEuropean Southern Observatory, Karl-Schwarzschild-str. 2, 85748 Garching bei München, GermanyA. MarconiDipartimento di Fisica e Astronomia, Universitá di Firenze, via G. Sansone 1, 50019 Sesto F.no, Firenze, ItalyN. MenciINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyR. MaiolinoCavendish Laboratory, University of Cambridge, 19 J. J. Thomson Ave., Cambridge CB3 0HE, UKE. PiconcelliINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyG. VietriINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, ItalyL. ZappacostaINAF–Osservatorio Astronomico di Roma, via Frascati 33, 00078 Monteporzio Catone, Italy
2017en
ABI
Аннотация
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.
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