Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE - The diverse ionization mechanisms acting in low-mass starbursts

Open Access

Fig. 7.

Emission line ratio maps of Haro 14. Top left: balmer decrement, Hα/Hβ. Top right: ratio of the collisional excited sulfur lines, [S II] λλ6717, 6731. Bottom left: excitation map, [O III] λ5007/Hβ. Bottom right: excitation map, [O III] λ5007/Hα. The contour levels of the Hα flux map are overplotted.

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