2019A&A...630A.111B


Query : 2019A&A...630A.111B

2019A&A...630A.111B - Astronomy and Astrophysics, volume 630A, 111-111 (2019/10-1)

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

BRUNI G., PICONCELLI E., MISAWA T., ZAPPACOSTA L., SATURNI F.G., VIETRI G., VIGNALI C., BONGIORNO A., DURAS F., FERUGLIO C., TOMBESI F. and FIORE F.

Abstract (from CDS):


Context. The WISSH quasars project aims at studying the nuclear and host galaxy properties of the most luminous quasars (Lbol>1047erg/s, 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 (≥2000km/s) 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 SiIV 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 (∼4000km/s) and maximum velocity (∼17000km/s). Moreover, for two objects we discovered BAL features bluewards of the SiIV peak, which can be associated with CIV 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.

Abstract Copyright: © ESO 2019

Journal keyword(s): galaxies: active - galaxies: nuclei - quasars: absorption lines - ISM: jets and outflows - quasars: general - quasars: supermassive black holes

CDS comments: Paragraph 3.5 1421+46 not identified (probable misprint)

Simbad objects: 40

goto Full paper

goto View the references in ADS

Number of rows : 40
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 [VV2006] J004527.7+143815 QSO 00 45 27.6880548528 +14 38 16.136609676   18.23 17.72     ~ 35 1
2 [VV2006] J021646.9-092107 QSO 02 16 46.9448340672 -09 21 07.301012184   19.57 18.73     ~ 32 0
3 2MASS J04142091+0609141 QSO 04 14 20.9059894104 +06 09 14.286637332           ~ 8 0
4 QSO J0747+2739 QSO 07 47 11.1466907592 +27 39 03.365989812     17.20     ~ 68 0
5 [VV2006] J092819.2+534023 QSO 09 28 19.2793363128 +53 40 24.123535464   23.75 21.86     ~ 28 0
6 2MASS J09473420+1421168 QSO 09 47 34.1970129912 +14 21 16.944191676   17.89 17.65     ~ 35 0
7 QSO J0959+1312 QSO 09 59 37.1146924200 +13 12 15.467765616   19.65 18.55     ~ 48 0
8 QSO B1010+5630 QSO 10 13 36.3797768496 +56 15 36.410820264   20.10 19.14     ~ 45 0
9 2MASS J10254174+2454243 QSO 10 25 41.7827456928 +24 54 24.277162680   20.10 19.89     ~ 19 0
10 QSO J1048+4407 QSO 10 48 46.6283653104 +44 07 10.856369964   23.89 21.80     ~ 37 0
11 QSO J1051+3107 QSO 10 51 22.4674763160 +31 07 49.420074540           ~ 29 0
12 QSO J1103+1004 QSO 11 03 52.7442282696 +10 04 03.182969352   20.45 19.58     ~ 38 0
13 2MASS J11101712+1930124 QSO 11 10 17.1368475312 +19 30 12.509090928           ~ 14 0
14 QSO B1107+4847 QSO 11 10 38.6370859200 +48 31 15.691679076   17.09 16.87     ~ 87 0
15 2MASS J11225878+1645405 QSO 11 22 58.7764854576 +16 45 40.348120644   18.82 18.37     ~ 18 0
16 QSO B1127+078 QSO 11 30 17.3821660536 +07 32 13.029808812   17.92 17.70     ~ 39 0
17 2MASS J11574799+2724595 QSO 11 57 47.9892554664 +27 24 59.656490100   19.70 18.99     ~ 17 0
18 2MASS J12044715+3309384 QSO 12 04 47.1499698000 +33 09 38.745290664   21.82 20.49     ~ 35 0
19 2MASS J12102762+1741088 QSO 12 10 27.6305128008 +17 41 08.836358424   21.23 19.98     ~ 13 0
20 QSO J1215-0034 QSO 12 15 49.8117265224 -00 34 32.172841452   17.76 17.51     ~ 81 0
21 SDSS J123714.60+064759.5 QSO 12 37 14.6105371632 +06 47 59.612187624   19.66 19.15     ~ 60 0
22 LBQS 1243+0121 QSO 12 45 51.4514622408 +01 05 05.025409332   18.43 18.26     ~ 64 0
23 SDSS J125050.88+204658.7 QSO 12 50 50.8846896600 +20 46 58.749482352   21.67 20.80     ~ 14 0
24 QSO J1305+0521 QSO 13 05 02.2779755136 +05 21 51.162622020   21.21 20.09     ~ 34 0
25 [VV2006] J132655.0-000531 QSO 13 26 54.9527826240 -00 05 30.134926968   21.22 20.81     ~ 35 0
26 [VV2006] J132827.1+581836 QSO 13 28 27.0686827248 +58 18 36.913458960   18.67 18.67     ~ 41 0
27 [VV2006] J142243.0+441721 QSO 14 22 43.0262924160 +44 17 21.323456196   19.96 19.08     ~ 38 0
28 SDSS J144709.24+103824.5 QSO 14 47 09.2457273672 +10 38 24.553025772           ~ 15 0
29 2MASS J14512531+1441361 QSO 14 51 25.3142854944 +14 41 36.018172644   18.64 18.30     ~ 13 0
30 QSO J1506+5220 QSO 15 06 54.5506795824 +52 20 04.744002588   21.72 20.14     ~ 56 0
31 QSO B1511+091 QSO 15 13 52.5256082976 +08 55 55.726612572   18.22 17.92     ~ 63 1
32 QSO J1538+0855 QSO 15 38 30.5596599072 +08 55 17.150004552   18.77 17.98     ~ 34 0
33 [VV2006] J154446.3+412035 QSO 15 44 46.3426267128 +41 20 35.701415124   20.88 19.67     ~ 31 0
34 2MASS J15493872+1245092 QSO 15 49 38.7147322320 +12 45 09.161026308   19.21 18.54 17.61   ~ 38 0
35 SDSS J155514.85+100351.3 QSO 15 55 14.8568584608 +10 03 51.279329952   21.02 20.00     ~ 18 0
36 [VV2006] J163300.1+362904 QSO 16 33 00.1384440000 +36 29 04.887068172   20.09 19.15     ~ 33 0
37 2MASS J16390910+2824471 QSO 16 39 09.1106351400 +28 24 47.164862052   19.61 18.48     ~ 34 0
38 SDSS J165053.78+250755.4 QSO 16 50 53.7837720504 +25 07 55.414503084           ~ 14 0
39 SDSS J212329.46-005052.9 QSO 21 23 29.4639412848 -00 50 52.916363736   16.91 16.62     ~ 119 0
40 2MASS J22380807-0808422 QSO 22 38 08.0788090680 -08 08 42.127798992   20.01 19.48     ~ 24 0

To bookmark this query, right click on this link: simbad:objects in 2019A&A...630A.111B and select 'bookmark this link' or equivalent in the popup menu