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Table 4

Line ratios measured for the different apertures/regions and for the different kinematic components.

Aperture Region Comp BPT/VO87 Class

[NII]/Hα [OI]/Hα [SII]/Hα
(1) (2) (3) (4) (5) (6) (7)

Ap-a Outflow-W N1 S2 S2 S2 S2
N2 S2 S2 S2 S2
B S2 S2 L/S2 S2:

Ap-d Outflow-E N1 S2/H ... H/S2 Cp
N2 S2 S2 S2 S2
I S2 S2/L L/S2 Cp

Ap-b S-Bubble N S2 S2 S2 S2
I1 S2 S2 S2 S2
I2 S2 S2/L S2 S2:

Ap-h N-Bubble N H/Comp H/S2 H Cp
I S2 S2 S2/L S2:
B S2 L/S2 L/S2 Cp

Ap-c SE compact N S2 S2/L S2/L Cp
B S2 S2/L S2/L Cp

Ap-j Ext. filaments N S2 S2 S2 S2

Notes. Column (1): extraction aperture. Column (2): corresponding region covered by the extraction aperture. Column (3): kinematic component. Columns (4)–(6): optical spectral type for each of the diagnostic diagrams. The symbols are: H = HII galaxies, L = LINER and S2 = Seyfert 2. Column (7): adopted optical spectral type. Cp indicates a mix between S2 and LINER and/or HII spectral types. Following Yuan et al. (2010) notation, single colons indicate apertures with the same spectral classification in two of the diagnostic diagrams.

(⋆)

For the broad component in these two apertures we assumed an Hα to Hβ ratio of 3. Therefore, the [OIII]/Hβ line ratios calculated are lower limits of the real values.

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