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Table C.3.

Peak flux of detected molecular emission measured within a circular 10″ aperture centered on the C-type semi-regular and irregular stars.

Line Frequency Peak flux [Jy]
[GHz] TW Oph NP Pup TW Hor T Ind RT Cap AQ Sgr U Hya W Ori V Aql Y Pav X Vel Y Hya SS Vir W CMa
Band 6, spectral window 1
SiO (5–4) 217.105 0.3 0.1 0.1 0.1 3.6 0.4 0.1 0.3 0.4
13CN (N = 2–1) (a) 217.287 0.1
13CN (N = 2–1) (b) 217.315 0.1 0.1
Band 6, spectral window 2
13CN (N = 2–1) (c) 217.467 0.1
SiS (12–11) 217.818
HC3N (24–23) 218.325 0.1 0.2 0.1 0.1 0.2
C4H (N = 23–22) (d) 218.837
C4H (N = 23–22) (e) 218.875
Band 6, spectral window 4
13CS (5–4) 231.221 0.1 0.1 0.1 0.1
29SiS (13–12) 231.627
SiC2 (102, 9–92, 8) 232.534 0.2 0.3 0.4 0.2 0.6
Band 7, spectral window 1
13CO (3–2) 330.588 0.8 0.2 4.5 0.4 0.4 0.7 0.3
SiC2 (146, 9–136, 8) 330.870 0.4 0.4 0.5 0.3 0.7
Band 7, spectral window 3
SiC2 (152, 14–142, 13) 342.805 0.3 0.1 0.5 0.4 0.3
CS (7–6) 342.883 3.4 1.6 0.3 1.1 5.0 6.2 3.6 4.5
29SiO (8–7) 342.981 0.1
Band 7, spectral window 4
13CN (4–3) 345.340 0.8 0.8 0.3 4.0 1.9 1.5 0.5 0.3 1.2 0.1

Notes. The spectral resolution for each spectral window is given in Sect. 3. The peak flux error is on the order of 20%.

(a)

J = 5/2 − 3/2, F1 = 2 − 1, F = 2 − 2;

(b)

J = 5/2 − 3/2, F1 = 2 − 2, F = 2 − 3;

(c)

J = 5/2 − 3/2, F1 = 3 − 2, F = 4 − 3;

(d)

J = 47/2 − 45/2, F = 23 − 22;

(e)

J = 45/2 − 43/2, F = 23 − 22.

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