Context. The WISSH quasars project aims at studying the nuclear and host galaxy properties of the most luminous quasars (Lbol > 1047 erg s-1, 1.8 < z < 4:6), with special emphasis on the occurrence and physical parameters of winds at different scales. Aims. Nuclear winds are manifested as UV-broad (≥2000 km s-1) absorption lines (BAL) in about 15% of quasars. We aim at studying the incidence and properties of such winds in the WISSH sample to investigate possible differences to active galactic nucleus regimes with lower luminosity. Methods. We collected optical spectra from the Sloan Digital Sky Survey (SDSS) data release 12, and identified those showing absorption troughs in the region between the Si iv and Civ emission lines. We used three different indices for BAL absorption: the classic balnicity index (BI), the absorption index (AI), and the intermediate AI1000. Results.We find a higher observed fraction of Civ BAL quasars in the WISSH sample (24%) than in previous catalogues (10-15%). These WISSH BAL quasars are also characterised by a higher average BI (∼4000 km s-1) and maximum velocity (∼17 000 km s-1). Moreover, for two objects we discovered BAL features bluewards of the Si iv peak, which can be associated with C iv absorption with a velocity of 0:15c. We also updated previous studies on the dependence of maximum outflow velocity upon bolometric luminosity, showing that BAL winds have intermediate properties compared to molecular or ionised winds and ultra-fast outflows. Finally, the radio properties of the WISSH BAL quasars as a whole are in line with those of samples at lower luminosities from previous studies. Conclusions. Our results suggest that the higher Lbol of the WISSH quasars likely favours the acceleration of BAL outflows and that their most likely driving mechanism is radiation pressure. Furthermore, we estimate that the kinetic power associated with these winds in hyperluminous quasars for the highest column density and fastest winds is sufficient to provide efficient feedback onto the host galaxy.

The WISSH quasars project: VI. Fraction and properties of BAL quasars in the hyper-luminosity regime

Vignali C.
Membro del Collaboration Group
;
2019

Abstract

Context. The WISSH quasars project aims at studying the nuclear and host galaxy properties of the most luminous quasars (Lbol > 1047 erg s-1, 1.8 < z < 4:6), with special emphasis on the occurrence and physical parameters of winds at different scales. Aims. Nuclear winds are manifested as UV-broad (≥2000 km s-1) absorption lines (BAL) in about 15% of quasars. We aim at studying the incidence and properties of such winds in the WISSH sample to investigate possible differences to active galactic nucleus regimes with lower luminosity. Methods. We collected optical spectra from the Sloan Digital Sky Survey (SDSS) data release 12, and identified those showing absorption troughs in the region between the Si iv and Civ emission lines. We used three different indices for BAL absorption: the classic balnicity index (BI), the absorption index (AI), and the intermediate AI1000. Results.We find a higher observed fraction of Civ BAL quasars in the WISSH sample (24%) than in previous catalogues (10-15%). These WISSH BAL quasars are also characterised by a higher average BI (∼4000 km s-1) and maximum velocity (∼17 000 km s-1). Moreover, for two objects we discovered BAL features bluewards of the Si iv peak, which can be associated with C iv absorption with a velocity of 0:15c. We also updated previous studies on the dependence of maximum outflow velocity upon bolometric luminosity, showing that BAL winds have intermediate properties compared to molecular or ionised winds and ultra-fast outflows. Finally, the radio properties of the WISSH BAL quasars as a whole are in line with those of samples at lower luminosities from previous studies. Conclusions. Our results suggest that the higher Lbol of the WISSH quasars likely favours the acceleration of BAL outflows and that their most likely driving mechanism is radiation pressure. Furthermore, we estimate that the kinetic power associated with these winds in hyperluminous quasars for the highest column density and fastest winds is sufficient to provide efficient feedback onto the host galaxy.
Bruni G.; Piconcelli E.; Misawa T.; Zappacosta L.; Saturni F.G.; Vietri G.; Vignali C.; Bongiorno A.; Duras F.; Feruglio C.; Tombesi F.; Fiore F.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11585/741772
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