A fast ionised wind in a star-forming quasar system at z ~ 1.5 resolved through adaptive optics assisted near-infrared data

Author： Brusa M.   Perna M.   Cresci G.   Schramm M.   Delvecchio I.   Lanzuisi G.   Mainieri V.   Mignoli M.   Zamorani G.   Berta S.   Bongiorno A.   Comastri A.   Fiore F.   Kakkad D.   Marconi A.   Rosario D.   Contini T.   Lamareille F.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|588|issue|A58-A58

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.588, Iss.issue, 2016-03, pp. : A58-A58

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Abstract

Aims. Outflow winds are invoked in co-evolutionary models to link the growth of SMBH and galaxies through feedback phenomena, and from the analysis of both galaxies and active galactic nuclei (AGN) samples at z ~ 1−3, it is becoming clear that powerful outflows may be very common in AGN hosts. High-resolution and high S/N observations are needed to uncover the physical properties of the wind through kinematics analysis.

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