Transition | Freq. | L1157-B1 | IRAS 16293 | OMC2-IRAS 4 | AFGL 2591 | NGC 6334I | |||||
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(GHz) | K km s-1 | km s-1 | K km s-1 | km s-1 | K km s-1 | km s-1 | K km s-1 | km s-1 | K km s-1 | km s-1 | |
H2O: 110-101 | 556.936 | 14.75(0.33) | 11.6 | 17.62(0.49) | 6.8 | 17.26(0.57) | 8.8 | 3.35(0.46) | 3.0 | ![]() |
- |
H2O: 532-441 | 620.701 | ![]() |
- | 1.80(0.18) | 9.9 | ![]() |
- | ![]() |
- | 5.15(0.52)a | 8.8 |
HDO: 211-202 | 599.927 | ![]() |
- | 0.73(0.23) | 4.6 | ![]() |
- | ![]() |
- | 1.67(0.45) | 6.8 |
CO: 5-4 | 576.268 | 54.20(0.32) | 4.8 | 87.78(1.82) | 9.7 | 147.59(0.74) | 11.3 | 165.52(0.93) | 7.8 | 133.63(9.63)a | 4.2 |
C17O: 5-4 | 561.713 | ![]() |
- | 2.46(0.32) | 2.9 | 1.09(0.17) | 2.2 | 4.28(0.57) | 3.4 | 15.47(0.89) | 4.6 |
HCO+: 7-6 | 624.208 | 0.11(0.03) | - | 17.70(0.18) | 2.4 | 16.87(0.18) | 4.1 | 9.99(0.40) | 3.8 | 32.36(1.24) | 5.9 |
H13CO+: 7-6 | 607.175 | ![]() |
- | 0.68(0.24) | 3.0 | ![]() |
- | ![]() |
- | 4.12(3.60) | 5.0 |
HCN: 7-6 | 620.304 | 0.96(0.13) | 7.4 | 5.45(0.16) | 5.2 | 16.87(0.38) | 8.9 | 2.66(0.28) | 3.7 | 21.39(0.70) | 8.0 |
H13CN: 7-6 | 604.268 | ![]() |
- | 0.57(0.14) | 6.0 | 0.77(0.11) | 12.3 | ![]() |
- | 6.81(0.43)b | 12.9 |
DCN: 8-7 | 579.205 | ![]() |
- | 0.29(0.12) | 6.0 | ![]() |
2.5 - | ![]() |
- | 1.2(4.38)b | 4.2 |
HNC: 7-6 | 634.510 | ![]() |
- | 0.58(0.17) | 3.8 | 0.35(0.20) | 1.7 | ![]() |
- | 3.26(0.74) | 6.6 |
CN: 505-404 | 566.731 | ![]() |
- | ![]() |
- | 1.77(0.10) | 6.1 | 0.79(0.25) | 3.2 | 4.13(1.49) | 7.8 |
CN: 506-405 | 566.947 | ![]() |
- | ![]() |
- | 1.39(0.19) | 3.4 | 0.98(0.26) | 3.0 | 4.12(1.38) | 5.8 |
N2H+: 6-5 | 558.967 | ![]() |
- | 0.45(0.15) | 1.9 | 6.84(0.12) | 2.2 | ![]() |
- | 11.87(1.77) | 4.5 |
NH3: 1,00-0,01 | 572.497 | 1.26(0.09) | 7.6 | 2.8(0.15)b | 3.5 | 8.32(0.14) | 4.5 | 3.52(0.27) | 4.2 | 7.79(0.66) | 3.8 |
HClc: 1-0 | 625.902 | ![]() |
- | 2.24(0.15) | 2.0 | 0.42(0.14) | 2.2 | 2.05(0.30) | 3.1 | 20.06(1.34)b | 18.5 |
H37Clc:1-0 | 624.978 | ![]() |
- | 0.76(0.18) | 1.5 | 0.28(0.12) | 4.1 | ![]() |
- | 5.63(3.09) | 13.4 |
CCH: 78-67 | 611.265 | ![]() |
- | ![]() |
- | 0.78(0.13) | 2.8 | ![]() |
- | 2.15(1.06) | 7.2 |
CCH: 77-66 | 611.328 | ![]() |
- | ![]() |
- | 0.84(0.15) | 3.9 | ![]() |
- | 1.33(1.15) | 6.1 |
H2CO: 818-717 | 561.899 | 0.63(0.11) | 4.4 | 4.21(0.18) | 4.2 | 6.61(0.16) | 4.3 | ![]() |
- | 9.98(0.59) | 6.5 |
H2CO: 808-707 | 576.708 | 0.39(0.11) | 7.9 | 2.00(0.10) | 4.5 | 2.65(0.10) | 4.2 | ![]() |
- | 7.13(0.48) | 7.1 |
H2CO: 827-726 | 581.612 | ![]() |
- | 1.19(0.11) | 5.2 | 1.53(0.12) | 4.1 | ![]() |
- | 4.40(0.52) | 5.3 |
H2CO: 854-753 | 582.382 | ![]() |
- | 0.51(0.15) | 6.2 | 0.79(0.14) | 3.4 | ![]() |
- | 3.16(0.38) | 5.7 |
H2CO: 835-734 | 583.309 | ![]() |
- | 1.57(0.14) | 4.9 | 2.01(0.12) | 3.9 | ![]() |
- | 5.39(0.83) | 5.9 |
H2CO: 826-725 | 587.454 | ![]() |
- | 1.18(0.14) | 4.9 | 1.18(0.12) | 3.7 | ![]() |
- | 4.05(0.45) | 4.8 |
H2CO: 817-716 | 600.331 | 0.19(0.04) | 8.2 | 3.43(0.19) | 4.3 | 5.11(0.14) | 4.6 | ![]() |
- | 8.79(0.50) | 6.7 |
H2CO: 819-718 | 631.703 | 0.44(0.11) | 3.8 | 3.41(0.15) | 4.4 | 5.08(0.14) | 4.4 | ![]() |
- | 8.14(0.69) | 6.4 |
H2S: 642-633 | 567.080 | ![]() |
- | ![]() |
- | ![]() |
- | ![]() |
- | 1.46(0.73) | 9.2 |
H2S: 331-322 | 568.051 | ![]() |
- | 0.48(0.13) | 4.5 | ![]() |
- | ![]() |
- | 3.40(0.50) | 5.0 |
H2S: 550-541 | 579.795 | ![]() |
- | ![]() |
- | ![]() |
- | ![]() |
- | 2.84(0.50) | 5.2 |
H2S: 532-523 | 611.442 | ![]() |
- | 0.40(0.14) | 6.4 | ![]() |
- | ![]() |
- | 1.98(0.72) | 6.4 |
CS: 12-11 | 587.616 | 0.19(0.03) | 5.2 | 3.18(0.17) | 4.2 | 4.10(0.14) | 10.9 | 0.92(0.28) | 4.5 | 15.13(0.49) | 6.7 |
C34S: 12-11 | 578.216 | ![]() |
- | 0.42(0.11) | 5.4 | ![]() |
- | ![]() |
- | 8.68(0.50) | 7.7 |
C34S: 13-12 | 626.349 | ![]() |
- | 0.40(0.14) | 5.0 | ![]() |
- | ![]() |
- | 3.92(0.69) | 5.4 |
SO: 1312-1211 | 558.087 | ![]() |
- | 2.77(0.14) | 5.2 | ![]() |
- | ![]() |
- | 3.55(0.33) | 4.9 |
SO: 1313-1212 | 559.319 | ![]() |
- | 2.88(0.14) | 5.4 | ![]() |
- | ![]() |
- | 3.64(0.35) | 5.6 |
SO: 1314-1213 | 560.178 | ![]() |
- | 3.12(0.17) | 5.1 | ![]() |
- | 0.76(0.22) | 4.4 | 4.83(0.37) | 6.6 |
SO: 1413-1312 | 601.258 | ![]() |
- | 2.53(0.14) | 5.5 | ![]() |
- | 0.92(0.24) | 5.4 | 2.89(0.52) | 5.0 |
SO: 1414-1313 | 602.292 | ![]() |
- | 2.25(0.21) | 5.1 | ![]() |
- | ![]() |
- | 2.28(0.69) | 4.3 |
SO: 1415-1314 | 603.021 | ![]() |
- | 2.84(0.13) | 5.5 | ![]() |
- | ![]() |
- | 3.94(0.38) | 5.6 |
SO2: 551-440 | 555.666 | ![]() |
- | 0.77(0.22) | 4.1 | ![]() |
- | ![]() |
- | ![]() |
- |
SO2: 15610-15511 | 560.891 | ![]() |
- | 0.49(0.12) | 8.3 | ![]() |
- | ![]() |
- | 0.69(0.33) | 3.6 |
SO2: 1368-1359 | 561.266 | ![]() |
- | ![]() |
- | ![]() |
- | ![]() |
- | 2.49(0.39)b | 5.2 |
SO2: 1166-1157 | 561.491 | ![]() |
- | ![]() |
- | ![]() |
- | ![]() |
- | 1.02(0.38) | 6.1 |
SO2: 1064-1055 | 561.560 | ![]() |
- | ![]() |
- | ![]() |
- | ![]() |
- | 0.86(0.55) | 5.0 |
SO2: 1148-1037 | 567.593 | ![]() |
- | 0.61(0.10) | 4.7 | ![]() |
- | ![]() |
- | 1.00(0.31) | 4.4 |
SO2: 651-542 | 574.807 | ![]() |
- | 0.72(0.10) | 4.2 | ![]() |
- | ![]() |
- | 1.31(0.26) | 5.9 |
SO2: 1248-1139 | 587.568 | ![]() |
- | 0.69(0.14) | 5.5 | ![]() |
- | ![]() |
- | 2.15(1.92) | 7.0 |
SO2: 753-642 | 593.945 | ![]() |
- | 0.60(0.12) | 3.9 | ![]() |
- | ![]() |
- | 0.66(0.58) | 3.3 |
SO2: 13410-1239 | 604.367 | ![]() |
- | 0.88(0.11) | 5.9 | ![]() |
- | ![]() |
- | 1.16(0.34) | 4.2 |
SO2: 853-744 | 613.076 | ![]() |
- | 0.62(0.12) | 4.1 | ![]() |
- | ![]() |
- | 1.33(0.62) | 5.9 |
SO2: 14410-13311 | 626.087 | ![]() |
- | 0.56(0.15) | 4.4 | ![]() |
- | ![]() |
- | ![]() |
- |
SO2: 955-844 | 632.193 | ![]() |
- | 0.63(0.16) | 4.2 | ![]() |
- | ![]() |
- | 1.63(0.47) | 5.1 |
Notes. The CH3OH lines detected in at least a
source other than NGC 6334I are reported in Table 4. Note
that we did not report the list of CH3OCH3 lines
as they are detected in NGC 6334I only and are the focus of a
forthcoming paper. For each source, we report the main beam temperature
integrated intensity
(K km s-1), and the FWHM
(km s-1)
obtained by fittting the line with a gaussian. In parenthesis we report
the rms over the same integration interval of the line intensity. Only
lines with rms larger than 3 are considered detected, except in
the case of NGC 6334I, where 1
was taken since the rms is artificially higher because of the line-crowed spectrum. Upper limits refer to 1
.
(a) Line is heavily absorbed; (b) line is merged; (c) only the central component.
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