Table 7: Comparison of average values of colour gradients for our full sample and for the Pec subsample of morphologically peculiar objects (Michard & Prugniel 2004). Among Pec objects we distinguish the YP family with evidence for the presence of some young stars and the NP family with no such evidence.
Y All N $A\rm v$ YP N $A\rm v$ NP N $A\rm v$
$\Delta _{BV}$ All 53 - $0.066\pm.003$ YP 9 $-0.060\pm.005$ NP 7 $-0.057\pm.006$
$\Delta _{UB}$ id 41 - $0.157\pm.007$ id 7 $-0.137\pm.006$ id 6 $-0.138\pm.010$
$\Delta_{BR}$ id 43 - $0.082\pm.004$ id 8 $-0.074\pm.005$ id 6 $-0.074\pm.011$
$\Delta_{VI}$ id 47 - $0.061\pm.005$ id 7 $-0.052\pm.006$ id 7 $-0.053\pm.008$
$\Delta _{VJ}$ id 53 - $0.136\pm.013$ id 9 $-0.108\pm.029$ id 7 $-0.123\pm.021$
$\Delta _{VK}$ id 53 - $0.227\pm.015$ id 9 $-0.169\pm.029$ id 7 $-0.201\pm.024$
$\Delta_{JK}$ id 54 - $0.093\pm.004$ id 9 $-0.073\pm.009$ id 7 $-0.083\pm.009$
(1) Gradient Y; (2) sample; (3) number of objects N; (4) average with estimated error; (5) sample; (6) number of objects N; (7) average with estimated error; (8) sample; (9) number of objects N; (10) average with estimated error.

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