Open Access

Table B.4

Number of COMs detected, from Yang et al. (2021), and detection of sulfur-bearing species toward each source.

Source COMs CS SO 34SO SO2 Class
Per-emb 13 16 0
Per-emb 12 B 15 0
Per-emb 29 14 0
Per-emb 44 14 I
Per-emb 27 14 0
B1-bS 9 0
Per-emb 26 9 0
Per-emb 17 9 0
Per-emb 11 A 7 0
Per-emb 35 A 5 I
Per-emb 33 A 3 0
Per-emb 18 3 0
L1448 IRS 3A 3 0
SVS 13B 3 0
Per-emb 22 B 2 0
Per-emb 22 A 2 0
Per-emb 20 2 0
Per-emb 35 B 2 I
Per-emb 12 A 2 0
Per-emb 5 2 0
Per-emb 1 2 0
Per-emb 42 1 I
Per-emb 21 1 0
Per-emb 2 1 0
Per-emb 10 1 0
Per-emb 11 C 1 0
Per-emb 53 1 I
SVS 13 A2 a 1 0/I?
L1448 NW 0 0
Per-emb 33 B/C 0 0
Per-emb 25 0 0
L1455 IRS2 0 I
Per-emb 36 0 0
Per-emb 54 0 I
Per-emb 15 0 0
Per-emb 50 0 I
IRAS 4B2 0 0
Per-emb 14 0 0
Per-emb 37 0 0
Per-emb 40 0 I
B1-bN 0 0
Per-emb 16 0 0
Per-emb 28 0 0
Per-emb 11 B 0 0
Per-emb 55 0 I
Per-emb 8 0 0
Per-emb 60 0 I
EDJ2009-172 0 I
EDJ2009-235 0 I
Per-emb 41 b ? ? ? ? ? I

Notes. (a)Source with unknown Tbol but, given the clustered nature, we could speculate that it is a protostar. (b)Source at the edge of the field of view.

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