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Table 4.

Average line ratios of the ionised gas for all the derived components.

Galaxy Component log([S II]/Hα) log([N II]/Hα) log([O I]/Hα) log([O III]/Hβ)
(1) (2) (3) (4) (5) (6)
NGC 0266 Primary 0.22 ± 0.19 0.42 ± 0.17 −0.68 ± 0.30
NGC 0315 Primary 0.28 ± 0.21 0.53 ± 0.18 −0.43 ± 0.33
Secondary 0.34 ± 0.31 0.13 ± 0.36 −0.23 ± 0.30
NGC 3226 Primary 0.06 ± 0.12 −0.04±0.09 −1.08 ± 0.19
Secondary 0.05 ± 0.25 0.17 ± 0.16 −0.60 ± 0.49
NGC 3245 Primary −0.30 ± 0.12 0.01 ± 0.01
Secondary −0.55 ± 0.24 −0.21 ± 0.15
NGC 4278 Primary 0.18 ± 0.12 0.17 ± 0.09 −0.18 ± 0.28
Secondary 0.17 ± 0.03 0.17 ± 0.04 0.35 ± 0.30
NGC 4438 Primary 0.05 ± 0.19 0.15 ± 0.15 −0.96 ± 0.49
Secondary 0.10 ± 0.12 0.16 ± 0.11 −1.10 ± 0.49
Tertiary 0.28 ± 0.16 0.25 ± 0.06
NGC 4750 Primary 0.07 ± 0.14 0.30 ± 0.13 −1.08 ± 0.55 −0.15 ± 0.33
Secondary 0.23 ± 0.16 0.42 ± 0.18 −0.80 ± 0.47
NGC 5055 Primary −0.23 ± 0.03 −0.09 ± 0.03

Notes. Columns indicate: (1) object; (2) kinematical component from the emission lines used to derived the ratios; (3–6) are the average line ratios in logarithm scale, considering the standard deviation as the 1σ error.

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