Fig. 4
CO luminosity as a function of luminosity in different wavelength bands: Ba), FUVb), Hαc), Kd), FIRe), and 1.4 GHz f). Black and gray points and lines show subsample I and subsample II BCDs, respectively. Arrows indicate CO upper limits. Dashed and solid lines indicate linear fits to detected only and all (detected and non-detected) galaxies, respectively.
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