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Fig. 2.

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Color spatial pattern in Haro 14. Left: (V − I) color index map; bluer colors indicate the bluer (younger) SF regions and red corresponds to the redder (older) stars in the galaxy. The map is not corrected for the contribution of emission lines. Right: increment in the (V − I) color index due to the contribution of emission lines. The blue line roughly delineates the bluish but not ionizing stellar component unveiled in the color map and the black contour corresponds to ΔL(V − I) = 0.01.

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