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Table 1

Logarithms of the observed line ratios for the H ii regions identified in NGC 5427 (see Fig. 2).

log  Ratios:
Region [O iii]/Hβ [N ii]/Hα [S ii]/Hα [O iii]/[O ii] [O iii]/[N ii] [O iii]/[S ii] [N ii]/[S ii] [N ii]/[O ii] log  q Δ log  q 12 +log (O/H) Δlog (O/H)]

021 –0.501 –0.495 –0.664 –0.339 –0.462 –0.293 0.169 0.123 7.39 0.17 9.11 0.06
06 –0.769 –0.483 –0.736 –0.931 –0.743 –0.49 0.253 –0.188 7.37 0.29 9.16 0.06
08 –0.803 –0.494 –0.647 –1.017 –0.765 –0.613 0.153 –0.251 7.15 0.17 9.13 0.06
09 –0.489 –0.466 –0.619 –0.651 –0.48 –0.327 0.153 –0.172 7.35 9 0.01 9.11 0.01
10 –0.631 –0.46 –0.656 –0.911 –0.628 –0.431 0.197 –0.282 7.27 0.22 9.12 0.06
11 –0.906 –0.487 –0.654 –0.876 –0.709 0.167 7.27 0.00 9.18 0.01
12 –0.76 –0.474 –0.602 –1.146 –0.742 –0.615 0.128 –0.404 7.07 0.23 9.09 0.09
13 –0.828 –0.517 –0.597 –0.912 –0.767 –0.688 0.079 –0.145 7.09 0.03 9.12 0.02
14 –0.689 –0.445 –0.65 –0.968 –0.7 –0.496 0.204 –0.268 7.26 0.24 9.13 0.07
15 –0.45 –0.455 –0.56 –0.795 –0.451 –0.346 0.105 –0.343 7.21 0.09 9.06 0.03
16 –0.245 –0.49 –0.539 –0.648 –0.212 –0.163 0.049 –0.436 7.21 0.01 9.00 0.01
17 –0.113 –0.549 –0.527 –0.503 –0.02 –0.043 –0.023 –0.483 7.23 0.08 8.92 0.04
18 0.101 –0.615 –0.532 –0.596 0.26 0.177 –0.084 –0.856 7.16 0.07 8.80 0.04
19 –0.68 –0.461 –0.583 –0.925 –0.675 –0.554 0.121 –0.249 7.15 0.12 9.11 0.04
20 –0.542 –0.495 –0.602 –0.874 –0.504 –0.397 0.107 –0.37 7.17 0.13 9.07 0.04
21 –0.624 –0.49 –0.569 –1.052 –0.59 –0.512 0.078 –0.462 7.06 0.17 9.05 0.07
22 –0.529 –0.493 –0.534 –0.928 –0.492 –0.451 0.041 –0.436 7.06 0.09 9 9.03 0.04
23 –0.471 –0.453 –0.525 –0.836 –0.475 –0.403 0.072 –0.361 7.15 0.08 9.05 8 0.02
24 –0.38 –0.463 –0.509 –0.818 –0.373 –0.327 0.046 –0.445 7.13 0.07 9.02 0.03
25 –0.47 –0.457 –0.531 –0.917 –0.469 –0.395 0.074 –0.448 7.12 0.13 9.04 0.05
26 –0.413 –0.489 –0.591 –0.893 –0.381 –0.279 0.102 –0.512 7.17 0.18 9.02 0.07
27 –0.37 –0.508 –0.518 –0.785 –0.318 –0.309 0.01 –0.466 7.09 0.03 8.99 0.02
28 –0.39 –0.49 –0.56 –0.871 –0.356 –0.287 0.07 –0.515 7.13 0.14 9.01 0.06
29 –0.41 –0.498 –0.543 –0.87 –0.368 –0.324 0.045 –0.502 7.10 0.10 9.00 0.05
301 –0.276 –0.439 –0.461 –1.06 –0.293 –0.272 0.021 –0.767 7.02 0.23 8.93 0.13
31 –0.234 –0.508 –0.494 –0.708 –0.183 –0.196 –0.014 –0.525 7.12 0.01 8.96 0.01
32 –0.852 –0.494 –0.679 –1.079 –0.814 –0.63 0.184 –0.265 7.18 0.24 9.14 0.08
33 –0.663 –0.531 –0.664 –0.815 –0.588 –0.456 0.133 –0.226 7.22 0.07 9.11 0.03
34 –0.602 –0.364 –0.561 –0.864 –0.694 –0.497 0.197 –0.17 7.30 0.17 9.14 0.04
351 –0.468 –0.469 –0.612 –1.32 –0.456 –0.313 0.143 –0.864 7.08 0.45 8.97 0.22
36 –0.405 –0.45 –0.534 –0.866 –0.411 –0.327 0.084 –0.455 7.15 0.14 9.03 0.05
37 –0.323 –0.524 –0.548 –0.695 –0.255 –0.231 0.024 –0.441 7.15 0.01 0 9.00 0.01
38 –0.112 –0.526 –0.535 –0.628 –0.042 –0.033 0.009 –0.585 7.20 0.03 8.94 0.02
39 –0.255 –0.507 –0.552 –0.749 –0.205 –0.16 0.045 –0.544 7.16 0.08 8.79 0.04

Notes.The mean ionisation parameters, log q = log (cU), where c is the speed of light in cm s-1, and the mean total oxygen abundances, 12 +log (O/H) are derived from the pyqz program (see text).

(1)

Region of low signal to noise or nuclear contaminated region not used in the abundance gradient analysis.

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