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Table D.4

Abundances in Class 0/I protostars from Perseus.

Source H2S H233S${\rm{H}}_{\rm{2}}^{{\rm{33}}}{\rm{S}}$ OCS OC33S OC34S SO(a) SO2(a) TOTAL(b) DS
×10–9 ×10–9 ×10–9 ×10–9 ×10–9 ×10–9 ×10–9 ×10–9
BlbN 1.442 0.025 0.0 0.0 0.0 <0.007 <0.029 1.464 l×l04
BlbS 16.03 0.036 1.741 0.031 0.077 <0.005 <0.019 17.78 8×l02
B5-IRS1 89.98 0.0 12.77 0.0 0.0 [0.307-0.950] <0.590 103.8 l×l02
HH211MMS 0.586 0.0 4.453 0.051 0.198 [0.034-0.100] [0.035-0.279] 5.263 3×l03
IC348MMS 41.88 0.083 2.803 0.025 0.125 >0.011 [0.005-0.030] 44.72 3×l02
IRAS2A >207.1 >0.411 67.16 0.495 2.985 >0.608 >0.970 >276.3 < 5×101
IRAS2B 1.142 0.0 1.173 0.0 0.0 >0.367 [0.070-0.828] 3.642 4×l03
IRAS4B 84.13 0.167 5.871 0.062 0.261 >0.013 [0.021-0.196] 90.12 2×l02
IRAS4C 0.379 0.0 <0.128 0.0 0.0 [0.059-0.179] <0.066 0.688 2×l04
L1448-IRS3A 1.383 0.0 13.74 0.149 0.611 >0.198 [0.111-1.003] 16.12 9×l02
L1448-IRS3B 0.537 0.0 3.195 0.016 0.142 [0.015-0.048] <0.045 3.793 4×l03
L1448C 4.113 0.0 12.01 0.093 0.534 >0.198 [0.201-3.133] 18.12 8×l02
L1448NW 0.275 0.0 <0.097 0.0 0.0 >0.045 [0.013-0.120] 0.518 3×l04
Per-emb-02 0.240 0.0 0.022 0.0 0.0 [0.015-0.040] <0.068 0.330 5×l04
Per-emb-05 0.206 0.0 2.658 0.010 0.118 [0.031-0.091] <0.090 2.986 5×l03
Per-emb-08 0.501 0.0 <0.126 0.0 0.0 [0.016-0.042] <0.064 0.697 2×l04
Per-emb-18 1.271 0.0 16.73 0.108 0.744 >0.201 [0.093-0.681] 18.76 8×l02
Per-emb-22 2.683 0.0 1.676 0.0 0.0 [0.024-0.164] [0.014-0.173] 4.527 3×l03
Per-emb-29 65.55 0.209 20.18 0.258 0.897 >0.063 [0.033-0.744] 85.93 6×101
Per-emb-30 0.0 0.0 0.0 0.0 0.0 0.0
Per-emb-50 0.0 0.0 0.0 0.0 0.0 > 1.108 [0.434-7.437] >6.408 <2×l03
Per-emb-62 0.0 0.0 0.0 0.0 0.0 0.0
SVS13A >1343 >6.139 392.2 3.542 17.43 >1.885 >2.686 >1742 <8.6
SVS13B 0.232 0.0 1.204 0.017 0.053 [0.019-0.078] <0.190 1.589 9×l03

Notes. (a) Retrieved from Artur de la Villarmois et al. (2023); no data from Per-emb-30 and Per-emb-62 (not observed).(b) Total abundance has been calculated using all lower and upper limits, and using the mean value of SO and SO2 in the cases a range is given. Lower and upper limits to the total sulfur abundance have only been explicited when a limit was given for the most abundant species in the source.

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