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Table 5

Isotope ratios of 34S/36S and 32S/36S.

Source RGC 34S/36S 32S/36S


(kpc) J = 2−1 J = 3−2 J = 2−1 J = 3−2
W3OH 9.64± 0.03 140±16 174 ± 29(*) 4181 ± 531 5195 ± 919(*)
Orion-KL 8.54 ± 0.00 92 ± 53 (*) 83±7 1954 ± 1207(*) 1765 ± 414
+20 km s−1 cloud 0.03 ± 0.03 69 ± 11(*) 1015 ± 278(*)
+50 km s−1 cloud 0.02 ± 0.04 41 ± 4 884 ± 104
G024.78+00.08 3.51 ± 0.15 151 ± 39(*) 226 ± 66(*) 2424 ± 699(*) 3640± 1164(*)
G030.81−00.05 5.73 ± 0.24 55 ± 15(*) 829 ± 233(*)
W51-IRS2 6.22 ± 0.06 109± 27(*) 203 ± 45(*) 1814 ± 506(*) 3397 ± 855(*)
DR21 8.10 ± 0.00 117 ± 24 159± 64(*) 3223 ± 742 4384 ± 1829(*)
NGC7538 9.47 ± 0.07 109 ± 28 (*) 2912 ± 897(*)

Below are the isotope ratios of 34S/36S and 32S/36S from Mauersberger et al. (1996)

W3OH 9.64± 0.03 181 ± 49 4118 ± 1124
Orion-KL 8.54 ± 0.00 104±7 2281 ± 174
IRAS15491 (**) 5.48 ± 0.31 108±15 2120 ± 307
IRAS15520 (**) 5.67 ± 0.31 128 ± 32 133 ± 11 2531 ± 641 2629 ± 243
IRAS16172 (**) 5.03 ± 0.29 121 ± 18 119±14 2334 ± 361 2296 ± 287
NGC6334A 6.87 ± 0.12 108±15 154± 20 2232 ± 322 3183 ± 431
NGC6334B 6.87 ± 0.12 163 ± 46 156 ± 26 3369 ± 960 3225 ± 552
W51(M) 6.22 ± 0.004 105 ± 11 104± 15 2119 ± 237 2099 ± 313

Notes. (*)Values with large uncertainties are derived from the tentative detection of C36S lines. (**)For these three sources without parallax data, their kinematic distances were estimated (for details, see Sect. 2.1). The 34S/36S and 32S/36S isotope ratios in this work from the J = 2−1 transition are corrected for the optical depth effects, while the ones for the 3−2 line could not be corrected.

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