2021ApJ...920...30N

Query : 2021ApJ...920...30N

2021ApJ...920...30N - Astrophys. J., 920, 30-30 (2021/October-2)

The picture of BLR in 2.5D FRADO: dynamics and geometry.

NADDAF M.-H., CZERNY B. and SZCZERBA R.

Abstract (from CDS):

The dynamics of the broad line region (BLR) in active galaxies is an open question; direct observational constraints suggest a predominantly Keplerian motion, with possible traces of inflow or outflow. In this paper we study in detail the physically motivated BLR model of Czerny & Hryniewicz based on the radiation pressure acting on dust at the surface layers of the accretion disk (AD). We consider here a nonhydrodynamical approach to the dynamics of the dusty cloud under the influence of radiation coming from the entire AD. We use here a realistic description of the dust opacity, and we introduce two simple geometrical models of the local shielding of the dusty cloud. We show that the radiation pressure acting on dusty clouds is strong enough to lead to dynamical outflow from the AD surface, so the BLR has a dynamical character of a (mostly failed) outflow. The dynamics strongly depends on the Eddington ratio of the source. Large Eddington ratio sources show a complex velocity field and large vertical velocities with respect to the AD surface, while for lower Eddington ratio sources vertical velocities are small and most of the emission originates close to the AD surface. Cloud dynamics thus determines the 3D geometry of the BLR.

Journal keyword(s): Galaxy accretion disks - Radiative processes - Broad-absorption line quasar - Quasars - Astrophysical dust processes - Gas-to-dust ratio - Active galactic nuclei - Active galaxies - Reverberation mapping - Supermassive black holes - Galaxy winds - Dust continuum emission

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	Z 296-15	Sy1	14 36 22.0820611632	+58 47 39.394934844		14.19	13.79			~	592	0

Query : 2021ApJ...920...30N

Basic data :

Z 296-15 -- Seyfert 1 Galaxy

G (2016A&A,Mrk,...), X (2012ApJS,2MAXI,...), AGN (2021Sci,[HB91],...), IR (IRAS,PSCz,...), Sy1 (2013ApJS), QSO (2016ApJ,QSO), rG (2018AJ), MIR (WISEA,WISE), EmG (2024A&A), * (Gaia), Rad (WN), UV (PG), NIR (2MASS), Opt (SDSS), var (2021Sci)

14 36 22.0820611632 +58 47 39.394934844 (Optical) [ 0.0151 0.0151 90 ] A 2020yCat.1350....0G

14 34 57.8885028241 +59 00 38.950533882 [ 0.0151 0.0151 90 ]

100.2997104169546 +53.4782797716016 [ 0.0151 0.0151 90 ]

0.018 -0.036 [0.019 0.018 90] A 2020yCat.1350....0G

V(km/s) 9207 [150] / z(emission) 0.03119806 [0.0005] / cz 9352.9431 [150] (Opt) C 2022ApJS..261....2K

Sr... D 2010AJ....139.2525H

0.66332 0.601631 163 (Opt) B 2023ApJS..269....3M

B 14.19 [~] D 2010A&A...518A..10V

V 13.79 [~] D 2010A&A...518A..10V

G 14.383773 [0.005187] C 2020yCat.1350....0G

J 11.784 [0.023] C 2006AJ....131.1163S

H 10.971 [0.026] C 2006AJ....131.1163S

K 10.346 [0.022] C 2006AJ....131.1163S

u (AB) 14.810 [0.004] B 2011yCat.2306....0A

g (AB) 14.130 [0.002] B 2011yCat.2306....0A

r (AB) 13.688 [0.002] B 2011yCat.2306....0A

i (AB) 13.463 [0.002] B 2011yCat.2306....0A

z (AB) 13.297 [0.003] B 2011yCat.2306....0A

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`Mrk 817`	`QSO B1434+5900`	`UGC 9412`	`[PVK2003] 219.09292 +58.79472`
`IRAS F14349+5900`	`1RXP J143622.9+584737`	`UZC J143622.1+584739`	`[VV2000c] J143622.1+584740`
`IRAS 14349+5900`	`RX J1436.3+5847`	`WISEA J143622.08+584739.4`	`[VV2003c] J143622.1+584740`
`LEDA 52202`	`1RXS J143622.2+584750`	`WISE J143622.09+584739.5`	`[VV2006c] J143622.1+584740`
`2MASS J14362207+5847394`	`SBSG 1434+590`	`WN B1434+5900`	`[VV2010c] J143622.1+584740`
`2MASX J14362213+5847389`	`SDSS J143622.07+584739.3`	`Z 296-15`	`[VV98c] J143622.1+584740`
`2MAXI J1437+588`	`SDSS J143622.09+584739.5`	`Z 1434.9+5901`	`[ZEH2003] RX J1436.3+5847 2`
`PBC J1436.3+5848`	`SDSS J143622.08+584739.4`	`[BAG2012] 219.1769+58.7837`	`Gaia DR3 1617151089269670016`
`PG 1434+590`	`SWIFT J1436.4+5846`	`[DML87] 350`	`Gaia DR2 1617151089269670016`
`PSCz Q14349+5900`	`SWIFT J1436.5+5847`	`[FS2003] 0717`
`QSO J1436+5847`	`TIC 298163846`	`[HB91] 1434+590`

References (592 between 1850 and 2026) (Total 592)
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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Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : Z 296-15

Link by name to the catalogue in VizieR :

`IRAS F14349+5900`	`IRAS 14349+5900`	`2MASS J14362207+5847394`	`2MASX J14362213+5847389`	`PG 1434+590`
`1RXS J143622.2+584750`	`SDSS J143622.07+584739.3`	`SDSS J143622.09+584739.5`	`SDSS J143622.08+584739.4`	`UGC 9412`
`WISEA J143622.08+584739.4`	`WISE J143622.09+584739.5`	`WN B1434+5900`	`[DML87] 350`	`Gaia DR3 1617151089269670016`
`Gaia DR2 1617151089269670016`

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