Clumps detected in Haro 14. Top-left: the 29 sources (clumps) detected in continuum (see also Table 3) overplotted on the blue (5400–5600 Å) continuum map. There is an evident clustering of the clumps at the galaxy eastern regions. Top-right: zoom into the central 20″ × 20″. The flux units are arbitrary. Bottom-left: the 55 clumps detected in emission lines (see also Table 4) overplotted on the Hα map; sources detected in Hα and [O III] λ5007 appear in blue, sources detected only in Hα in cyan, and those detected only in [O III] λ5007 in green. Bottom-right: zoom into the central galaxy regions. The intensity scale is logarithmic and the cross marks the position of the continuum peak.