Understanding the star formation efficiency in dense gas: Initial results from the CAFFEINE survey with ArTéMiS

Open Access

Fig. 12

Cumulative SFE above $N_{H_{2}}$ ${N_{{{\rm{H}}_2}}}$ > 2.8 × 10²² cm⁻² against the 90th percentile of FUV flux over the region observed by CAFFEINE. The red line indicates the SFE predicted by the filament scenario and the green line shows the result of a fitted power-law with a slope of −0.05 ± 0.05 and a p-value of 0.34.

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