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Table 5

Predicted abundances (with respect to H2) of selected molecules.

Species TE at rs Modelled at rs Modelled at 6R Observed Reference

CO 1.0 × 10-3 7.3 × 10-4 7.4 × 10-4 2.0 × 10-4 Decin et al. (2010b)
3.0 × 10-4 Kim et al. (2010)

H2O 2.1 × 10-4 1.1 × 10-4 1.8 × 10-4 6.6 × 10-5 Decin et al. (2010b)

SiO 9.5 × 10-5 6.4 × 10-5 1.9 × 10-5 8.0 × 10-6 Decin et al. (2010b)
5.1 × 10-6–1.3 × 10-5 Kim et al. (2010)

SiS 4.0 × 10-8 2.2 × 10-7 2.7 × 10-7 1.1 × 10-5 Decin et al. (2010a)
3.1 × 10-7–1.3 × 10-6 Kim et al. (2010)
1.0 × 10-7 Schoïer et al. (2007)

SO 4.3 × 10-8 2.1 × 10-12 7.3 × 10-8 4.0 × 10-7 Decin et al. (2010a)
2.7 × 10-7–7.8 × 10-7 Kim et al. (2010)

SO2 1.3 × 10-11 1.8 × 10-14 4.3 × 10-9 2.0 × 10-6 Decin et al. (2010a)
4.2 × 10-6–1.4 × 10-5 Kim et al. (2010)
1.7 × 10-8–3.7 × 10-7 a Yamamura et al. (1999)

HCN 6.3 × 10-12 7.7 × 10-7 5.0 × 10-8 1.3 × 10-7 Schoïer et al. (2013)
4.3 × 10-7–1.4 × 10-6 Kim et al. (2010)
4.4 × 10-7 Decin et al. (2010b)

CS 1.9 × 10-11 2.5 × 10-6 5.7 × 10-7 8.0 × 10-8 Decin et al. (2010b)
8.1 × 10-8–3.0 × 10-7 Kim et al. (2010)

PN 4.0 × 10-10 5.7 × 10-7 5.8 × 10-7 3.0 × 10-7 De Beck et al. (2013)

PO 1.0 × 10-7 3.3 × 10-10 2.0 × 10-10 5.4 × 10-8–6.0 × 10-7 De Beck et al. (2013)

NaCl 3.7 × 10-12 7.8 × 10-10 1.0 × 10-8 4.0 × 10-9 Milam et al. (2007)

NH3 1.1 × 10-11 2.8 × 10-9 1.5 × 10-19 1–3 × 10-6 Menten et al. (2010)

CO2 4.1 × 10-8 2.5 × 10-8 4.4 × 10-9 5.9 × 10-8 b Markwick et al. (2000)
2 × 10-9–4 × 10-8 a Yamamura et al. (1999)
AlO 8.0 × 10-9 2.6 × 10-8 1.6 × 10-10 3.4 × 10-8 c Kamiński et al. (2013a)
AlOH 4.5 × 10-9 4.5 × 10-6 1.5 × 10-6 1.0 × 10-7 c Tenenbaum & Ziurys (2010)
TiOd 2.4 × 10-7 1.8 × 10-7 1.8 × 10-7 5.0 × 10-9 c Kamiński et al. (2013b)
TiO2 1.3 × 10-12 6.2 × 10-10 4.8 × 10-9 6.3 × 10-10 c Kamiński et al. (2013b)
3.8 × 10-8 c De Beck et al. (2015)
HCl 3.5 × 10-7 3.9 × 10-7 3.7 × 10-7 1.5 × 10-8 e Yamamura et al. (2000)
AlCl 1.5 × 10-10 3.8 × 10-12 2.2 × 10-10 < 5 × 10-8 c Tenenbaum & Ziurys (2010)
SH 2.8 × 10-6 1.3 × 10-7 2.3 × 10-8 2.0 × 10-7 e Yamamura et al. (2000)
H2S 8.1 × 10-8 2.8 × 10-5 1.0 × 10-8 < 2 × 10-6 e Yamamura et al. (2000)

Notes.

(a)

SO2 & CO2 abundances derived from data of T Cephei.

(b)

The [CO2]/[H2O] ratio as measured in R Cas was used to estimate CO2 abundance in IK Tau.

(c)

Measured in the supergiant VY Canis Majoris.

(d)

Also detected in the inner wind of the S star NP Aurigae by Smolders et al. (2012).

(e)

Measured at 1.1 R in the S star R Andromedae.

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