2020A&A...641A.114H

Query : 2020A&A...641A.114H

2020A&A...641A.114H - Astronomy and Astrophysics, volume 641A114-114 (2020/9-1)

The ablation of gas clouds by blazar jets.

HEIL J. and ZACHARIAS M.

Abstract (from CDS):

Context. Flaring activity in blazars can last for vastly different timescales, and it may be the result of density enhancements in the jet flow that result from the intrusion of an interstellar cloud into the jet.
Aims. We investigate the lightcurves expected from the ablation of gas clouds by the blazar jet under various cloud and jet configurations.
Methods. We derived the semi-analytical formulae describing the ablation process of a hydrostatic cloud and performed parameter scans of artificial set-ups over both cloud and jet parameter spaces. We then used parameters obtained from measurements of various cloud types to produce lightcurves of these cloud examples.
Results. The parameter scans show that a vast zoo of symmetrical lightcurves can be realized. Both cloud and emission region parameters significantly influence the duration and strength of the flare. The scale height of the cloud is one of the most important parameters as it determines the shape of the lightcurve. In turn, important cloud parameters can be deduced from the observed shape of a flare. The example clouds result in significant flares lasting for various timescales.

Abstract Copyright: © ESO 2020

Journal keyword(s): radiation mechanisms: non-thermal - galaxies: active - galaxies: jets - gamma rays: galaxies

Simbad objects: 1

Full paper

View the references in ADS

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	4C 11.69	Bla	22 32 36.40890093	+11 43 50.9040592		17.75	17.33			~	1205	2

Query : 2020A&A...641A.114H

Basic data :

4C 11.69 -- Blazar

Rad (2014ApJS,4C,...), QSO (2010ApJ,QSO,...), gam (2AGL,2EG,...), Bla (2009A&A,RBPL,...), X (2009A&A,1E,...), AGN (2011ApJ), G (LEDA,[HSN2016]), * (USNO,Gaia), UV (GALEX,UVQS), MIR (WISEA,WISE), Q? (2021MNRAS), AG? (2022ApJS), NIR (2MASS)

22 32 36.40890093 +11 43 50.9040592 (Radio) [ 0.0327514 0.0375 0 ] A 2020A&A...644A.159C

22 30 07.81126892 +11 28 22.7077456 [ 0.0327514 0.0375 0 ]

077.43790775921 -38.58249241282 [ 0.0327514 0.0375 0 ]

-0.053 -0.044 [0.049 0.050 90] A 2020yCat.1350....0G

V(km/s) 183284 [150] / z(emission) 1.03624018 [0.0005] / cz 310656.9906 [150] (Opt) C 2022ApJS..261....2K

0.0263 [0.0357] A 2020yCat.1350....0G

B 17.75 [~] D 2010A&A...518A..10V

V 17.33 [~] D 2010A&A...518A..10V

G 15.961690 [0.055710] C 2020yCat.1350....0G

J 15.174 [0.045] C 2003yCat.2246....0C

H 14.556 [0.063] C 2003yCat.2246....0C

K 13.765 [0.052] C 2003yCat.2246....0C

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`4C 11.69`	`87GB 223008.3+112820`	`RGB J2232+117`	`[BDW2002] q2230+1128`
`2AGL J2232+1132`	`ICRF J223236.4+114350`	`RORF 2230+114`	`[CGL99] 24`
`BWE 2230+1128`	`IERS B2230+114`	`RX J2232.5+1143`	`[DGT2001] B2230+114`
`4C -11.69`	`INTREF 1082`	`RX J2232.6+1143`	`[GGR94] 2230+114`
`CLASS J223236.4110+114350.886`	`JVAS J2232+1143`	`1RXS J223236.8+114331`	`[HB93] 2230+114`
`CTA 102`	`JVAS B2230+114`	`S2 2230+11`	`[HSN2016] J338.15+11.73`
`Cul 2230+114`	`1Jy 2230+11`	`SQUAD DR1 J223236+114350`	`[IN88] 2230+114`
`DA 582`	`1Jy 2230+114`	`SWIFT J2232.3+1141`	`[LBD96] J2233+1140`
`1E 2230.1+1128`	`LEDA 2819036`	`SWIFT J2232.5+1141`	`[MGL2009] BZQ J2232+1143`
`2E 4622`	`2MASS J22323640+1143508`	`TGSSADR J223236.4+114350`	`[MML2015] 5BZQ J2232+1143`
`2E 2230.1+1128`	`MC2 2230+11.4`	`TIC 418977201`	`[P82] 2230+114`
`2EG J2233+1140`	`MITG J223236+1143`	`TXS 2230+114`	`[S77] 377`
`3EG J2232+1147`	`MRC 2230+114`	`USNO-A2.0 0975-20981161`	`[SBS92] 2230+114`
`EGR J2234+1127`	`NEWPS5 J2232+1143`	`UT 2230+114`	`[SJS95] 2230+114`
`0FGL J2232.4+1141`	`NVSS J223236+114350`	`UVQS J223236.41+114350.8`	`[VV2000] J223236.4+114351`
`1FGL J2232.5+1144`	`OHIO Y 150`	`VLSSr J223236.5+114347`	`[VV2003] J223236.4+114351`
`2FGL J2232.4+1143`	`PBC J2232.4+1144`	`VLSS J2232.6+1143`	`[VV2006] J223236.4+114351`
`3FGL J2232.5+1143`	`PCCS2 143 G077.42-38.59`	`VSOP J2232+1143`	`[VV2010] J223236.4+114351`
`4FGL J2232.5+1143`	`PKS 2230+114`	`WB 2230+1128`	`[VV96] J223236.4+114351`
`4FGL J2232.6+1143`	`PKS J2232+1143`	`WISEA J223236.41+114350.8`	`[VV98] J223236.4+114351`
`3FHL J2232.7+1143`	`PKS 2230+11`	`WISE J223236.40+114350.9`	`[WCO2009] J223235+114250`
`FIRST J223236.3+114350`	`QSO B2230+1128`	`WMAP 47`	`[WTW94] 2230+114`
`FL8Y J2232.5+1143`	`QSO J2232+1143`	`WMAP J2232+1144`	`[ZEH2003] RX J2232.6+1143 2`
`1FLE J2231+1132`	`QSO B2230+114`	`WMAP J2232+1143`	`Gaia DR3 2730046556694317312`
`GALEX J223236.4+114351`	`RBPL J2232+1143`	`WMAP J2232+1142`	`Gaia DR2 2730046556694317312`
`GB6 B2230+1128`	`RFC J2232+1143`	`9Y-MST J2232+1143`
`GB6 J2232+1143`	`RGB J2232.6+1143`	`[ATZ98] F100`

References (1205 between 1850 and 2026) (Total 1205)
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 : 4C 11.69

Link by name to the catalogue in VizieR :

`4C 11.69`	`BWE 2230+1128`	`4C -11.69`	`2E 4622`	`3EG J2232+1147`
`FIRST J223236.3+114350`	`GALEX J223236.4+114351`	`IERS B2230+114`	`2MASS J22323640+1143508`	`MITG J223236+1143`
`NVSS J223236+114350`	`PKS 2230+114`	`PKS J2232+1143`	`PKS 2230+11`	`1RXS J223236.8+114331`
`USNO-A2.0 0975-20981161`	`VSOP J2232+1143`	`WISEA J223236.41+114350.8`	`WISE J223236.40+114350.9`	`WMAP J2232+1144`
`WMAP J2232+1143`	`WMAP J2232+1142`	`Gaia DR3 2730046556694317312`	`Gaia DR2 2730046556694317312`

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