Dust tori in radio galaxies | Astronomy & Astrophysics (A&A)

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Volume 511 (February 2010)

A&A, 511 (2010) A64

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Table 3:

Median values of important physical parameters for the different radio galaxy classes.
Class	N	z	$\log{\nu L^{{\rm core}}_{{\rm 5GHz}}}$	$\log{\nu L_{{\rm 408~MHz}}^{{\rm total}}}$	$\log{R}$	$\log{\nu L^{{\rm core}}_{{\rm 11.85}~\mu{\rm m}}}$	VISIR	$\log{L_{\rm {bol}}}$	$\log{M_{\rm {BH}}}$	$\log{\frac{L_{\rm {bol}}}{L_{\rm {Edd}}}}$
							Resolution
			( ${\rm erg}~{\rm s}^{-1}$ )	( ${\rm erg}~{\rm s}^{-1}$ )		( ${\rm erg}~{\rm s}^{-1}$ )	(parsec)	( ${\rm erg}~{\rm s}^{-1}$ )	( $M_{\odot}$ )
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)
All	27	0.05540	40.17	41.59	-1.92	42.94	450	42.5	8.5	-4.1
FR-I	8	0.02332	39.34	40.83	-1.48	<41.97	180	41.8	8.8	-5.1
LEG	6	0.09210	40.48	41.98	-1.86	<43.16	780	<42.3	8.3	<-4.2
HEG	7	0.08147	39.55	41.59	-2.20	<43.13	680	<42.5	8.5	-4.1
BLRG	6	0.07101	40.44	42.13	-1.89	44.18	590	45.1	8.5	-1.7

Source LaTeX | All tables | In the text

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