2023ApJ...953L..26R


Query : 2023ApJ...953L..26R

2023ApJ...953L..26R - Astrophys. J., 953, L26 (2023/August-3)

First Results from the JWST Early Release Science Program Q3D: Benchmark Comparison of Optical and Mid-infrared Tracers of a Dusty, Ionized Red Quasar Wind at z = 0.435.

RUPKE D.S.N., WYLEZALEK D., ZAKAMSKA N.L., VEILLEUX S., BERTEMES C., ISHIKAWA Y., LIU W., SANKAR S., VAYNER A., LIM H.X.G., McCRORY R., MURPHREE G., WHITESELL L., SHEN L., LIU G., BARRERA-BALLESTEROS J.K., CHEN H.-W., DIACHENKO N., GOULDING A.D., GREENE J.E., HAINLINE K.N., HAMANN F., HECKMAN T., JOHNSON S.D., LUTZ D., LUTZGENDORF N., MAINIERI V., NESVADBA N.P.H., OGLE P. and STURM E.

Abstract (from CDS):

The [O III] 5007 Å emission line is the most common tracer of warm, ionized outflows in active galactic nuclei across cosmic time. JWST newly allows us to use mid-IR spectral features at both high spatial and spectral resolution to probe these same winds. Here we present a comparison of ground-based, seeing-limited [O III] and space-based, diffraction-limited [S IV] 10.51 μm maps of the powerful, kiloparsec-scale outflow in the Type 1 red quasar SDSS J110648.32+480712.3. The JWST data are from the Mid-InfraRed Instrument. There is a close match in resolution between the data sets (∼0.″6), in ionization potential of the O+2 and S+3 ions (35 eV) and in line sensitivity (1-2 × 10–17 erg s–1 cm–2 arcsec–2). The [O III] and [S IV] line shapes match in velocity and line width over much of the 20 kpc outflowing nebula, and [S IV] is the brightest line in the rest-frame 3.5-19.5 μm range, demonstrating its usefulness as a mid-IR probe of quasar outflows. [O III] is nevertheless intrinsically brighter and provides better contrast with the point-source continuum, which is strong in the mid-IR. There is a strong anticorrelation of [O III]/[S IV] with average velocity, which is consistent with a scenario of differential obscuration between the approaching (blueshifted) and receding (redshifted) sides of the flow. The dust in the wind may also obscure the central quasar, consistent with models that attribute red quasar extinction to dusty winds.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Quasars - Galaxy winds

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 7C 110357.29+482338.00 QSO 11 06 48.3334856808 +48 07 12.243925200   19.52 18.94 17.95   ~ 34 1

Query : 2023ApJ...953L..26R

Basic data :
7C 110357.29+482338.00 -- Quasar
Other object types:
otypes_help
Rad (2012ApJ,7C,...), QSO (2017A&A), AGN ([VV2006c],[VV2010c]), Q? (F2M), * (Gaia), NIR (2MASS), Opt (SDSS)
ICRS coord. (ep=J2000) :
11 06 48.3334856808 +48 07 12.243925200 (Optical) [ 0.0894 0.1529 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
11 03 56.9103191114 +48 23 25.913673507 [ 0.0894 0.1529 90 ]
Gal coord. (ep=J2000) :
160.0122018520807 +60.7834784914785 [ 0.0894 0.1529 90 ]
Proper motions mas/yr :
-0.005 -0.083 [0.105 0.187 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 103800 [~] / z(spectroscopic) 0.435000 [~] / cz 130409.72 [~]
   (Opt) D 2018A&A...613A..51P
Parallaxes (mas):
0.0137 [0.1676] A 2020yCat.1350....0G
Fluxes (12) :
B 19.52 [~] D 2010A&A...518A..10V
V 18.94 [~] D 2010A&A...518A..10V
R 17.95 [~] D 2012ApJ...757...51G
G 18.239202 [0.003692] C 2020yCat.1350....0G
J 16.250 [0.098] C 2010AJ....139.2360S
H 15.118 [0.085] C 2010AJ....139.2360S
K 13.943 [0.051] C 2010AJ....139.2360S
u (AB) 20.1850 [0.0600] C 2020ApJS..250....8L
g (AB) 19.1275 [0.0219] C 2020ApJS..250....8L
r (AB) 18.3409 [0.0409] C 2020ApJS..250....8L
i (AB) 17.9043 [0.0181] C 2020ApJS..250....8L
z (AB) 17.4747 [0.0191] C 2020ApJS..250....8L
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Identifiers (16) :
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7C 110357.29+482338.00 ILT J110648.40+480712.4 SDSS J110648.32+480712.3 [VV2006c] J110648.3+480712
F2M J110648.35+480712.3 2MASS J11064835+4807121 TGSSADR J110648.3+480712 [VV2010c] J110648.3+480712
FIRST J110648.3+480712 NVSS J110648+480713 TIC 318360958 Gaia DR2 831673481467882240
ILT J110648.37+480712.1 SDSS J110648.34+480712.2 WN B1103.9+4823 Gaia DR3 831673481467882240

References (34 between 1850 and 2026) (Total 34)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 7    Plx : 1    PM : 2   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : 7C 110357.29+482338.00

Link by name to the catalogue in VizieR :

FIRST J110648.3+480712 2MASS J11064835+4807121 NVSS J110648+480713 SDSS J110648.34+480712.2 SDSS J110648.32+480712.3
WN B1103.9+4823 Gaia DR2 831673481467882240 Gaia DR3 831673481467882240

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