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Fig. 15
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Summary of the abundances with respect to H2 derived for the hot corino observed towards SVS13-A (Chen et al. 2009, 
= 3 × 1024 cm−2). Blue points are for the S-species reported in the present paper, while blue triangles (Bianchi et al. 2019a) and grey diamonds (Belloche et al. 2020) are for iCOMs (see Sect. 6.1).
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