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

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

doi:10.1051/0004-6361/201527900

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Volume 588 (April 2016)

A&A, 588 (2016) A58

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Table 1

Emission line properties in the integrated spectra.

	Coordinates	H	K	f_Hα	f_{[O III]}	f_{[O II] 3727}	z	λ	FWHM

Nucleus (integrated 1′′)
Narrow Component (NC)	10:02:58.39 +02:10:13.94	19.70	19.90	106 ± 13	151 ± 7	37 ± 2	1.4718 ± 0.0001	12 376.1	550 ± 20
Outflow Component (OC)^(a)	′′	′′	′′	147 ± 31	467 ± 6	51 ± 2	1.4695 ± 0.0001	12 352.9	1735 ± 35

NW plume (integrated 0.4′′)
Single Component	10:02:58.42 +02:10:14.4	23.90	25.30	33 ± 3	53± 6	....	1.4711 ± 0.0001	12 372.5	530 ± 15

SE source
Single Component	10:02:58.46 +02:10:13.2	22.06	21.38	< 20	< 10	...	...	....	500

Notes. All fluxes in 10^-17 erg/s/cm²; all velocities in km s^-1.

^(a)

The centroid of the OC profile is blueshifted of Δv = −272 ± 22 km s^-1.

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