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Table 3

Characteristics of observed lines.

Source Species Transition υlsr Tmba Δυb ∫ Tdυ σrms
(km s-1) (mK) (km s-1) (K km s-1) (mK)
IRAS 05358 + 3543 HDO J = 11,0 − 10,1 ... .. ... ... 20
HDO J = 32,1 − 22,1 ... ... ... ... 40
HO J = 31,3 − 22,0 ... ... ... ... 30
SO2 J = 120,12 − 111,11  −15.9(4) 90 6.6(5) 0.61(4) 30
IRAS 18089 − 1732 HDO J = 11,0 − 10,1 32.1(1) 130 4.5(3) 0.62(3) 10
HDO J = 32,1 − 22,1 32.7(1) 420 6.3(3) 2.8(1) 50
HO J = 31,3 − 22,0 32.7(2) 180 5.7(2) 1.09(7) 30
SO2 J = 120,12 − 111,11 32.9(4) 430 9.5(4) 4.4(1) 30
IRAS 18151 − 1208-MM1 HDO J = 11,0 − 10,1 ... ... ... ... 20
HDO J = 32,1 − 22,1 ... .. ... ... 50
HO J = 31,3 − 22,0 ... ... ... .. 40
SO2 J = 120,12 − 111,11 33.3(3) 80 4.2(8) 0.36(5) 40
IRAS 18151 − 1208-MM2 HDO J = 11,0 − 10,1 ... ... ... ... 20
HDO J = 32,1 − 22,1 ... .. ... ... 60
HO J = 31,3 − 22,0 ... ... ... .. 50
SO2 J = 120,12 − 111,11 ... ... ... ... 50
IRAS 18264−1152 HDO J = 11,0 − 10,1 ... ... ... .. 60
HDO J = 32,1 − 22,1 ... ... ... ... 330
HO J = 31,3 − 22,0 ... ... .. ... 290
SO2 J = 120,12 − 111,11 ... ... ... ... 290
W43-MM1 HDO J = 11,0 − 10,1 101.3(1) 107 5.7(2) 0.65(2) 20
HDO J = 32,1 − 22,1 100.4(1) 410 7.5(2) 3.24(9) 60
HO J = 31,3 − 22,0 100.6(5) 220 3.8(7) 1.1(3) 80
SO2 J = 120,12 − 111,11 100.7(3) 230 5.2(7) 1.29(6) 80
DR21(OH)-S HDO J = 11,0 − 10,1 ... ... ... ... 20
HDO J = 32,1 − 22,1 ... .. ... ... 30
HO J = 31,3 − 22,0 ... ... ... .. 40
SO2 J = 120,12 − 111,11  −3.5(1) 240 3.5(2) 0.87(3) 10
NGC 7538S HDO J = 11,0 − 10,1  −56.7(5) 20 6(1) 0.11(2) 20
HDO J = 32,1 − 22,1  −57.9(8) 20 10(2) 0.57(9) 50
HO J = 31,3 − 22,0 ... .. ... ... 50
SO2 J = 120,12 − 111,11  −55.7(1) 580 6.1(1) 3.71(5) 50
IRAS 23385 + 6053 HDO J = 11,0 − 10,1 ... ... ... ... 10
HDO J = 32,1 − 22,1 ... ... ... .. 60
HO J = 31,3 − 22,0 .. ... ... ... 30
SO2 J = 120,12 − 111,11  −50.3(6) 40 8(2) 0.35(5) 10

Notes. Lines are fitted with a single Gaussian profile. Numbers in brackets indicates the error bar associated with the last decimal written. DR21(OH) is not reported here, having its own dedicated table.

(a)

Conversion factor is S/Tmb = 4.95 Jy/K for IRAM 30 m telescope.

(b)

The line emission velocity width is measured at the full width half maximum (FWHM).

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