2015A&A...577A..37A


Query : 2015A&A...577A..37A

2015A&A...577A..37A - Astronomy and Astrophysics, volume 577A, 37-37 (2015/5-1)

Anatomy of the AGN in NGC 5548. II. The spatial, temporal, and physical nature of the outflow from HST/COS Observations.

ARAV N., CHAMBERLAIN C., KRISS G.A., KAASTRA J.S., CAPPI M., MEHDIPOUR M., PETRUCCI P.-O., STEENBRUGGE K.C., BEHAR E., BIANCHI S., BOISSAY R., BRANDUARDI-RAYMONT G., COSTANTINI E., ELY J.C., EBRERO J., DI GESU L., HARRISON F.A., KASPI S., MALZAC J., DE MARCO B., MATT G., NANDRA K.P., PALTANI S., PETERSON B.M., PINTO C., PONTI G., POZO NUNEZ F., DE ROSA A., SETA H., URSINI F., DE VRIES C.P., WALTON D.J. and WHEWELL M.

Abstract (from CDS):

AGN outflows are thought to influence the evolution of their host galaxies and of super massive black holes. Our deep multiwavelength campaign on NGC 5548 has revealed a new, unusually strong X-ray obscuration, accompanied by broad UV absorption troughs observed for the first time in this object. The X-ray obscuration caused a dramatic decrease in the incident ionizing flux on the outflow that produces the long-studied narrow UV absorption lines in this AGN. The resulting data allowed us to construct a comprehensive physical, spatial, and temporal picture for this enduring AGN wind. We aim to determine the distance of the narrow UV outflow components from the central source, their total column-density, and the mechanism responsible for their observed absorption variability. We study the UV spectra acquired during the campaign, as well as from four previous epochs (1998-2011). Our main analysis tools are ionic column-density extraction techniques, photoionization models based on the code CLOUDY, and collisional excitation simulations. A simple model based on a fixed total column-density absorber, reacting to changes in ionizing illumination, matches the very different ionization states seen in five spectroscopic epochs spanning 16 years. The main component of the enduring outflow is situated at 3.5±1.1pc from the central source, and its distance and number density are similar to those of the narrow-emitting-line region in this object. Three other components are situated between 5-70pc and two are farther than 100pc. The wealth of observational constraints and the anti-correlation between the observed X-ray and UV flux in the 2002 and 2013 epochs make our physical model a leading contender for interpreting trough variability data of quasar outflows. This campaign, in combination with prior UV and X-ray data, yields the first simple model that can explain the physical characteristics and the substantial variability observed in an AGN outflow.

Abstract Copyright:

Journal keyword(s): galaxies: Seyfert

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 - 2024
#notes
1 NGC 5548 Sy1 14 17 59.5400291832 +25 08 12.603122268   14.35 13.73     ~ 2710 0

Query : 2015A&A...577A..37A

Basic data :
NGC 5548 -- Seyfert 1 Galaxy
Origin of the objects types :

(Ref) Object type as listed in the reference "Ref"
(acronym) Object type linked to the acronym according to the original reference
() Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some particular cases

Other object types:
X (2A,3A,...), G (2015ApJ,ECO,...), AGN (2010ApJS,[HB91],...), UV (2EUVE,EUVE,...), MIR (AKARI,WISEA,...), IR (IRAS,PSCz,...), Sy1 (2013ApJS), QSO (2016ApJ,QSO), SyG (2013ApJS), EmG (2015A&A), GiC ([BKB95]), GiG ([CHM2007]), AG? (2020MNRAS), V* (AAVSO), * (Gaia), gam (INTREF), NIR (2MASS), Opt (SDSS), var (2021Sci)
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
ICRS coord. (ep=J2000) :
14 17 59.5400291832 +25 08 12.603122268 (Optical) [ 0.0242 0.0270 90 ] A 2020yCat.1350....0G
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
FK4 coord. (ep=B1950 eq=1950) :
14 15 43.4924015726 +25 22 01.249516687 [ 0.0242 0.0270 90 ]
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
Gal coord. (ep=J2000) :
031.9607439471738 +70.4957558374883 [ 0.0242 0.0270 90 ]
Syntax of proper motions is : "pm-ra pm-dec [error ellipse] quality bibcode"
  • pm-ra : mu-ra*cos(dec) (expressed in the ICRS system in mas/yr)
  • pm-dec : mu-dec (expressed in the ICRS system in mas/yr)
  • [error ellipse] : error major axis and minor axis (in mas), orientation angle (in deg)
  • quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the proper motion reference
Proper motions mas/yr :
-0.147 0.065 [0.032 0.032 90] A 2020yCat.1350....0G
Syntax of radial velocity (or/and redshift) is : "value [error] (wavelength) quality bibcode"
  • value : radial velocity or/and redshift (Heliocentric frame) according to your Output Options
    (redshift may be not displayed if the data value is <0 and the database inside value is a radial velocity)
  • [error] : error of the corresponding value displayed before
  • (wavelength) : wavelength range of the measurement : Rad, mm, IR, Opt, UV, Xray, Gam or  '∼'(unknown)
  • quality : flag of quality ( A=best quality -> E=worst quality, ∼=unknown quality)
  • bibcode : bibcode of the value's origin
Radial velocity / Redshift / cz :
V(km/s) 4961 [150] / z(emission) 0.01668582 [0.0005] / cz 5002.2830 [150]
   (Opt) C 2022ApJS..261....2K
Syntax of morphological type is : mtype quality bibcode
  • mtype : Hubble morphological class (spirals, ellipticals, etc)
  • quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the morphological type reference
Morphological type:
SA C 2019MNRAS.488..590B
Syntax of angular size is : "maj-axis min-axis angle (wtype) quality bibcode"
  • maj-axis : major axis size (arc minutes)
  • min-axis : minor axis size (arc minutes)
  • angle : orientation angle (in degrees)
  • (wtype) : wavelength class for the origin of the angular size (Rad, mm, IR, Opt, UV, Xray, Gam)
  • quality : flag of quality of the angular size values ( A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the angular size reference
Angular size (arcmin):
0.800 0.688 140 (NIR) C 2006AJ....131.1163S
Syntax of fluxes (or magnitudes) is : "filter-name (System) flux-value [error] quality MultVarFlags bibcode"
  • filter-name : U, B, V, R, I, G, J, H, K, u, g, r, i, z
  • (System) : may be AB (default is Vega)
  • flux-value : value of flux or magnitude
  • [error] : error value
  • quality : flag of quality of the flux value ( A=best quality -> E=worst quality, {� } =unknown quality)
  • MultVarFlags : Mult is zero or one char (J) for joined photometry ; Var can be zero or two chars (V[0-4])
  • bibcode : bibcode of the flux reference
Fluxes (11) :
B 14.35 [~] D 2010A&A...518A..10V
V 13.73 [~] D 2010A&A...518A..10V
G 14.398336 [0.010239] C 2020yCat.1350....0G
J 10.643 [0.018] C 2006AJ....131.1163S
H 9.884 [0.017] C 2006AJ....131.1163S
K 9.387 [0.019] C 2006AJ....131.1163S
u (AB) 14.812 [0.004] C 2009ApJS..182..543A
g (AB) 13.355 [0.002] C 2009ApJS..182..543A
r (AB) 12.626 [0.002] C 2009ApJS..182..543A
i (AB) 12.323 [0.002] C 2009ApJS..182..543A
z (AB) 12.058 [0.002] C 2009ApJS..182..543A
SIMBAD within arcmin
', {sourceSize:12, color:'#30a090'})); aladin.on('objectClicked', function(object) { var objName=object.data.MAIN_ID; aladin.showPopup(object.ra,object.dec,'',''+ objName+''); });" title="Show Simbad objects"> Overlay Simbad points in this preview
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 3
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%This number is the number of distinct objets linked, by using this button, you will obtain all links (may be more than one) from that object to his children

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: 3 Display criteria :

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Identifiers (62) :
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NGC 5548 LEDA 51074 SDSS J141759.54+250812.7 [CHM2007] LDC 1053 J141759.51+2508124
2A 1415+255 2MASS J14175955+2508126 SWIFT J1417.9+2507 [DML87] 344
3A 1415+253 2MASX J14175951+2508124 SWIFT J1418.2+2507 [HB91] 1415+253
AKARI-IRC-V1 J1417595+250812 2MAXI J1417+253 TIC 156602278 [KRL2007b] 154
2E 3236 MAXI J1418+251 4U 1414+25 [KVC2005] 3
2E 1415.7+2522 MCG+04-34-013 UGC 9149 [VV2000c] J141759.6+250813
ECO 4631 Mrk 1509 UVQS J141759.54+250812.6 [VV2003c] J141759.6+250813
2EUVE J1417+25.1 PBC J1417.9+2508 UZC J141759.6+250813 [VV2006c] J141759.6+250813
EUVE J1417+25.1 PSCz Q14156+2522 WISEA J141759.54+250812.6 [VV2010c] J141759.6+250813
1H 1415+255 QSO J1417+2508 WISE J141759.55+250812.7 [VV98c] J141759.6+250813
H 1416+256 RBS 1367 2XMM J141759.5+250812 [ZEH2003] RX J1418.0+2508 1
H 1415+253 1RXP J141759.3+250811 XSS J14181+2514 AAVSO 1413+25
INTREF 597 RX J141759+25081 Z 133-25 Gaia DR3 1255795527649038720
IRAS 14156+2522 RX J1418.0+2508 Z 1415.7+2522 Gaia DR2 1255795527649038720
IRAS F14157+2522 RX J1417.9+2508 [BKB95] 1415+2522
KUG 1415+253 1RXS J141759.6+250817 [CHM2007] HDC 866 J141759.51+2508124

References (2710 between 1850 and 2024) (Total 2710)
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


velocities : 27    distance : 3    PM : 2   

   

Observing logs


herschel : 4    ISO : 7    IUE : 258    XMM : 3   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : NGC 5548

Link by name to the catalogue in VizieR :

NGC 5548 AKARI-IRC-V1 J1417595+250812 2E 3236 EUVE J1417+25.1 IRAS 14156+2522
IRAS F14157+2522 KUG 1415+253 2MASS J14175955+2508126 2MASX J14175951+2508124 1RXS J141759.6+250817
SDSS J141759.54+250812.7 UGC 9149 WISEA J141759.54+250812.6 WISE J141759.55+250812.7 [DML87] 344
Gaia DR3 1255795527649038720 Gaia DR2 1255795527649038720

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