Fig. 10.
Molecular abundances with respect to methyl formate towards low-mass hot corinos (yellow): IRAS2A (Taquet et al. 2015) and IRAS4A2 in NGC 1333 (Taquet et al. 2015; López-Sepulcre et al. 2017), IRAS16293B (Jørgensen et al. 2016; Coutens et al. 2016; Lykke et al. 2017; Calcutt et al. 2018); the intermediate-mass protostars (red): Cep E-A (this work) and NGC 7129 (Fuente et al. 2014); the high-mass hot cores (blue): G29.96 (Beuther et al. 2009), Orion KL (Pagani et al. 2017; Beuther et al. 2009) and SgrB2(N1) (Belloche et al. 2013). Sources are ordered from left to right by increasing luminosity.
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