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Table C.2.

Peak flux of detected molecular emission measured within a circular 10″ aperture centered on the M-type Mira stars.

Line Frequency Peak flux [Jy]
[GHz] R Leo R Hya R Hor RR Aql IRC-10529 WX Psc IRC+10365
Band 6, spectral window 1
SiO (v = 1, J = 5–4) 215.596 36 6.0 0.5 0.3 2.5 17 4.0
34SO (65–54) 215.840 0.1 0.1 0.1 0.1
SO2 (222, 20–221, 21) 216.643 5.7 0.2
H2S (22, 0–21, 1) 216.710 0.3 0.2
SiS (v = 1, J = 12–11) 216.758 0.1
SiO (5–4) 217.105 36 22.4 6.7 4.2 5.7 9.6 12
Band 6, spectral window 2
SiS (12–11) 217.818 1.8 2.9 0.9
Band 6, spectral window 4
29SiS (13–12) 231.627 0.2 0.4 0.1
SO2 (v2 = 1, 143, 11–142, 12) 231.981
Si33S (13–12) 232.629 0.1
H2O (v2 = 1, 55, 0–64, 3) 232.687 0.3 0.1
Band 7, spectral window 1
13CO (3–2) 330.588 3.2 2.0 4.0 0.5 7.0 7.0 6.0
Na37Cl (27–26) 330.805 0.1
Band 7, spectral window 2
SO2 (116, 6–125, 7) 331.580
SO2 (212, 20–211, 21) 332.091 0.4 0.3
SO2 (43, 1–32, 2) 332.505 0.4 1.9 1.2 1.2 0.8
30SiS (19–18) 332.550 0.3 0.5 0.2
Band 7, spectral window 3
SO2 (343, 31–342, 32) 342.762 0.3
CS (7–6) 342.883 0.7 0.2 0.7 1.4 1.0
29SiO (8–7) 342.981 21.5 12.5 7.0 2.0 1.3 2.7 3.1
SiS (v = 1, J = 19–18) 343.101 0.3 0.4
SO (3Σv = 1, 98–87) 343.829
SO (88–77) 344.311 4 1.4 1.4 1.4 0.4 0.4 0.8
Band 7, spectral window 4
H13CN (4–3) 345.340 7.7 0.9 1.4 0.6 1.7 1.6

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

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