Fig. 8
Comparison of relative molecular abundances in FG0.89SW (from most to less abundant), diffuse clouds (Lucas & Liszt 2000a,b; Liszt & Lucas 2001; Lucas & Liszt 2002; Liszt et al. 2004), translucent clouds (Turner 2000), TMC-1 (Ohishi et al. 1992), Sgr B2(N) (Nummelin et al. 2000), LMC-N113 (Wang et al. 2009), and the nuclear region of the starburst galaxies NGC 253 (Martín et al. 2006) and NGC 4945 (Wang et al. 2004).
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