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Table 5

Oxygen abundances in the H ii regions in the disks of our sample of galaxies.

Slit R/R25 12+log(O/H)a Method Spectrum

NGC 1087

15 0.527 8.44 CNS red
16 0.359 8.48 CNS red
17 0.232 8.50 CNS red
23 0.050 8.61 CNS red
28 0.327 8.50 CNS red
30 0.506 8.52 CNS red
31 0.231 8.55 CNS red
32 0.444 8.42 CNS red
36 0.603 8.48 CNS red

NGC 2967

14 0.232 8.66 CNS red
17 0.554 8.53 CON blue
23 0.454 8.60 CNS red
28 0.575 8.45 CNS red
29 0.494 8.55 CNS red
33 0.936 8.35 CON blue
37 0.785 8.44 CNS red
39 0.949 8.36 CNS red

NGC 3023

08 0.449 8.16 Te blue
8.10 CNS red
12 0.336 8.16 Te blue
8.22 CNS red
14 0.110 8.34 C ON blue
8.30 C NS red
18 0.665 8.09 C NS red
19 0.575 8.22 C NS red
21 0.826 8.09 C NS red
22 1.117 7.99 C NS red

NGC 4030

46 0.910 8.52 C ON blue

NGC 4123

6 0.001 8.60 C NS red
14 0.528 8.54 C ON blue
18 0.711 8.47 C NS red
20 0.629 8.51 C ON blue
21 0.646 8.54 C ON blue
22 0.889 8.44 C NS blue
8.47 C ON blue
26 1.399 8.26 C ON blue

NGC 4517A

44 0.603 7.95 C ON blue
56 0.082 8.32 C ON blue

Notes.

(a)

Standard error for the C-based methods is around 0.1 dex. See Sect. 5.1 for more details.

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