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Table 8

Results of the analysis of the radial gradients of a set of properties.

Parameter Ngal rcor σr meda σa erra medb σb errb
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

μB 25 0.98 0.02 21.64 0.84 0.26 1.68 0.01 0.23
B − V 25 0.50 0.22 0.87 0.20 0.30 –0.20 0.15 0.27

rHII (100 pc) 11 0.61 0.24 2.57 0.25 0.30 –0.48 0.20 0.26
12 + log10(OH) 25 0.60 0.25 8.84 0.13 0.30 –0.12 0.11 0.27
log10( | EWHα | ) 25 0.57 0.21 0.95 0.32 0.25 0.51 0.28 0.22
log10( [NII] /Hα) 25 0.54 0.24 –0.41 0.13 0.30 –0.10 0.13 0.27
log10( [OIII] /Hβ 25 0.53 0.28 –0.59 0.32 0.25 0.29 0.26 0.22
log(U) 11 0.35 0.24 –3.93 0.29 0.04 0.09 0.12 0.08
ne (100 cm-3) 22 0.21 0.13 2.48 7.79 0.26 0.31 0.67 0.24
AV (mag) 25 0.17 0.17 1.60 0.88 0.25 –0.29 0.52 0.22

Notes. (1) Parameter which gradient is analyzed, eg., PARAM = a + b ∗ R/Re; (2) number of galaxies fulfilling the criteria (nHII > 30 regions); (3) median value of the derived correlation coefficients for the analyzed gradient; (4) standard deviation of the derived correlation coefficients; (5) median value for derived zero-points for each galaxy; (6) standard deviation of the derived zero-point; (7) median error of the derived zero-points; (8) median value of the derived slopes for each galaxy; (9) standard deviation of the derived slopes; (10) median error of the derived slopes.

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