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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