2001MNRAS.327..739G

Query : 2001MNRAS.327..739G

2001MNRAS.327..739G - Mon. Not. R. Astron. Soc., 327, 739-743 (2001/November-1)

Relativistic large-scale jets and minimum power requirements.

GHISELLINI G. and CELOTTI A.

Abstract (from CDS):

The recent discovery, by the Chandra satellite, that jets of blazars are strong X-ray emitters at large scales (0.1-1Mpc), lends support to the hypothesis that emitting plasma is still moving at highly relativistic speeds on these scales. In this case in fact the emission via inverse Compton scattering off cosmic background photons is enhanced and the resulting predicted X-ray spectrum accounts well for the otherwise puzzling observations. Here we point out another reason to favour relativistic large-scale jets, based on a minimum power argument: by estimating the Poynting flux and bulk kinetic powers corresponding to, at least, the relativistic particles and magnetic field responsible for the emission, one can derive the value of the bulk Lorentz factor for which the total power is minimized. It is found that both the inner and extended parts of the jet of PKS 0637-752 satisfy such a condition.

Abstract Copyright: The Royal Astronomical Society

Journal keyword(s): radiative mechanisms: non-thermal - galaxies: active - galaxies: jets

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	QSO J0635-7516	Bla	06 35 46.5079301472	-75 16 16.816418256		15.96	15.75	15.82		~	625	1

Query : 2001MNRAS.327..739G

Basic data :

QSO J0635-7516 -- Blazar

Rad (2014ApJS,CRATES,...), QSO (2008ApJS,QSO,...), X (2009A&A,1E,...), gam (1FGL,2FGL,...), Bla (2009A&A,[DGT2001],...), AGN (2011ApJ,CGRaBS), cm (AT20G,ATPMN), UV (PG,UVQS), MIR (WISEA,WISE), IR (IRAS,2MASSI), Sy1 (2013ApJS), rG (2023ApJS), Bz? (2013ApJS), Q? (2021MNRAS), AG? (2022ApJS), G (LEDA), * (Gaia), NIR (2MASS)

06 35 46.5079301472 -75 16 16.816418256 (Optical) [ 0.0238 0.0246 90 ] A 2020yCat.1350....0G

06 37 23.3905402210 -75 13 37.549370514 [ 0.0238 0.0246 90 ]

286.3683644283547 -27.1584170552254 [ 0.0238 0.0246 90 ]

0.026 0.051 [0.031 0.029 90] A 2020yCat.1350....0G

V(km/s) 139321 [150] / z(emission) 0.65420709 [0.0005] / cz 196126.3516 [150] (Opt) C 2022ApJS..261....2K

B 15.96 [~] D 2008MNRAS.384..775M

V 15.75 [~] D 2010A&A...518A..10V

R 15.82 [~] D 2008ApJS..175...97H

G 15.724110 [0.005312] C 2020yCat.1350....0G

J 14.846 [0.036] C 2003yCat.2246....0C

H 14.481 [0.058] C 2003yCat.2246....0C

K 13.632 [0.046] C 2003yCat.2246....0C

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`QSO J0635-7516`	`INTREF 309`	`RORF 0637-752`	`[BDW2002] q0637-7513`
`AT20G J063546-751616`	`IRAS F06374-7513`	`RX J0635.7-7516`	`[CGB93] 063723.3-751338`
`AT20G J063546.3-751616`	`IVS B0637-752`	`1RXS J063547.2-751617`	`[DGT2001] B0637-752`
`ATPMN J063546.4-751616`	`1Jy 0637-752`	`SPASS J063551-751600`	`[HB93] 0637-752`
`CGRaBS J0635-7516`	`1Jy 0637-75`	`SRGA J063545.9-751617`	`[MEM2008] 92`
`CRATES J063542-751615`	`LEDA 2824867`	`SUMSS J063544-751615`	`[MGL2009] BZQ J0635-7516`
`1E 0637.4-7513`	`2MASS J06354652-7516166`	`SUMSS J063545-751615`	`[MML2015] 5BZQ J0635-7516`
`2E 1720`	`2MASSI J0635465-751616`	`SWIFT J0635.9-7515`	`[VV2000] J063546.5-751617`
`2E 0637.4-7513`	`2MAXI J0634-751`	`SWIFT J0635.8-7514`	`[VV2003] J063546.5-751617`
`1ES 0637-75.2`	`MRC 0637-752`	`SWIFT J0636.1-7516`	`[VV2006] J063546.5-751617`
`1FGL J0636.1-7521`	`MSH 06-7-01`	`TIC 142107558`	`[VV2010] J063546.5-751617`
`2FGL J0635.5-7516`	`PBC J0635.4-7514`	`UVQS J063546.51-751616.7`	`[VV96] J063546.5-751617`
`3FGL J0635.7-7517`	`PCCS2 143 G286.37-27.15`	`VSOP J0635-7516`	`[VV98] J063546.5-751617`
`4FGL J0635.6-7518`	`PG 0637-752`	`WISEA J063546.51-751616.7`	`[WCO2009] J063536-751515`
`FL8Y J0635.6-7518`	`PKS 0637-752`	`WISE J063546.51-751616.9`	`[WTW94] 0637-752`
`G4Jy 618`	`PKS 0637-75`	`WISE J063546.51-751616.7`	`Gaia DR2 5261519281893469568`
`GLEAM J063547-751617`	`PKS J0635-7516`	`WMAP 167`	`Gaia DR3 5261519281893469568`
`ICRF J063546.5-751616`	`PMN J0635-7516`	`WMAP J0635-7517`	`Gaia DR1 5261519277596998912`
`IERS B0637-752`	`QSO B0637-7513`	`WMAP J0635-7516`
`IGR J06354-7516`	`QSO B0637-752`	`WMAP J0634-7514`

References (625 between 1850 and 2026) (Total 625)
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 : QSO J0635-7516

Link by name to the catalogue in VizieR :

`2E 1720`	`IERS B0637-752`	`IRAS F06374-7513`	`2MASS J06354652-7516166`	`2MASSI J0635465-751616`
`PG 0637-752`	`PKS 0637-752`	`PKS 0637-75`	`PKS J0635-7516`	`PMN J0635-7516`
`1RXS J063547.2-751617`	`SUMSS J063544-751615`	`SUMSS J063545-751615`	`VSOP J0635-7516`	`WISEA J063546.51-751616.7`
`WISE J063546.51-751616.9`	`WISE J063546.51-751616.7`	`WMAP J0635-7517`	`WMAP J0635-7516`	`WMAP J0634-7514`
`Gaia DR2 5261519281893469568`	`Gaia DR3 5261519281893469568`	`Gaia DR1 5261519277596998912`

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