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Table 6

Mid-IR luminosity of the sample targets, inferred bolometric luminosity, inner radii using Eq. (10) and “Barvainis radius” at 300 K as well as observed mid-IR half-light radius in pc.

Name log (LMIR/erg/s) log (Lbol/erg/s) r in r 300  K r 1/2
[pc] [pc] [pc]

I Zw 1 44.9 46.2 0.49 124 <2.7
NGC 424 43.6 44.7 0.09 23 1.3
NGC 1068 44.0 45.2 0.15 37 1.6 ± 0.1
NGC 1365 42.5 43.3 0.02 4.4 0.3 ± 0.1
IRAS 05189-2524 44.6 45.9 0.36 89 <3.5
H 0557-385 44.4 45.6 0.25 63 <1.6
IRAS 09149-6206 44.9 46.3 0.53 132 <2.7
MCG-05-23-16 43.5 44.6 0.08 19 1.9
Mrk 1239 44.0 45.2 0.15 38 0.8
NGC 3281 43.4 44.4 0.06 15 <0.6
NGC 3783 43.7 44.8 0.09 23 2.0
NGC 4151 43.0 44.0 0.04 9.4 >1.7
3C 273 45.7 47.2 1.54 387 8.1
NGC 4507 43.7 44.8 0.10 25 3.0
NGC 4593 43.1 44.1 0.04 11 ...
ESO 323-77 43.7 44.8 0.10 24 1.1 ± 0.2
Centaurus A 41.8 42.6 0.01 1.8 <0.05
IRAS 13349+2438 45.5 47.0 1.22 305 <6.2
IC 4329 A 44.2 45.4 0.19 47 <0.8
Circinus 42.7 43.6 0.03 6.4 0.8 ± 0.1
NGC 5506 43.4 44.4 0.06 16 <0.4
NGC 5995 44.1 45.2 0.16 50 <2.5
NGC 7469 43.9 45.0 0.12 30 4.0

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