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Fig. 21

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Star formation rate based on the FUV and 24    μm emission as a function of the molecular gas surface density. The crosses are based on X = 1020 cm-2 (K km s-1)-1, which is half of the Galactic value. The bridge region outside the giant Hii region near UGC 12915 are marked as squares with crosses. Squares without crosses correspond to a 2.5 times lower X factor as suggested by Zhu et al. (2007). Data of NGC 4438 are shown as triangles. The dashed lines correspond to constant star formation timescales of 2 and 4 Gyr.

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