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Fig. 1

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Relation between TS   iii and TO   iii temperatures inferred from the [S iii] and [O iii] auroral-to-nebular line ratios for the objects studied by PM06, including the three Hii galaxies later observed by H06. The light gray dashed line depicts the locus of equal temperatures (TS   iii = TO   iii), while the solid line indicates the error-weighted least-squares fit to the data (see Sect. 2).

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