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Table 6

Morphological classification, FIR colors, and compactness classification for the SBs of our sample.

Galaxy Morp. log f60/f100 log f25/f60 Comp.
class class

CGCG011-076 S –0.20 –0.89 3
CGCG043-099 S –0.19 –1.05 3
ESO148-IG002 CP 0.01 –0.82 2
ESO239-IG002 M –0.04 –0.79 2
ESO244-G012 CP –0.10 –0.68 2
ESO264-G036 S –0.34 –0.96 4
ESO286-IG019 M 0.07 –0.81 2
ESO440-IG058 P –0.23 –0.99 3
ESO507-G070 S –0.08 –1.21 1
IC 1623A/B CP –0.14 –0.80 2
IC 2545 M 0.01 –0.88 2
IC 2810 P –0.22 –1.00 3
IC 4687/6 P –0.13 –0.76 2
IRAS12224-0624 S –0.14 –1.48 1
IRAS14378-3651 S –0.08 –1.00 1
IRAS16399-0937 CP –0.24 –0.87 3
IRAS17207-0014 M –0.05 –1.36 1
IRAS18090+0130 P –0.31 –0.98 4
MCG-02-01-051/2 P –0.14 –0.79 2
MCG-03-04-014 S –0.15 –0.91 3
NGC 0034 M 0.01 –0.85 2
NGC 0232 P –0.23 –0.89 3
NGC 3110 P –0.30 –1.00 4
NGC 5010 S –0.33 –0.85 4
NGC 5331 CP –0.29 –1.0 0 4
NGC 6240 CP –0.06 –0.81 2
NGC 6926 S –0.31 –0.83 4
NGC 7130 P –0.19 –0.89 3
NGC 7592 CP –0.12 –0.92 2
NGC 7674 P –0.19 –0.45 2

Notes.Following Hattori et al. (2004), type 1 have SF region <500 pc, type 2 < 1 Kpc, type 3 > 1 Kpc and type 4 have extranuclear star formation.

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