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Table B.2
IRAM and HIFI 13CO, SiO and SiS line observations.
| Star | 13CO (1 → 0) | SiO (13 → 12) | SiS (6 → 5) |
| [K km s-1] | [K km s-1] | [K km s-1] | |
|
|
|||
| C Stars | |||
| R Scl | 4.7 (0.4) | <0.1 | <0.4 |
| V701 Cas | * 2.7 (0.2) | <0.22 | 0.94 (0.15) |
| V384 Per | 3.9 (0.2) | 0.73 (0.18) | 0.77 (0.14) |
| GY Cam | 2.0 (0.2) | <0.20 | 0.38 (0.15) |
| V1259 Ori | 3.5 (0.2) | <0.21 | 1.40 (0.13) |
| V688 Mon | * 1.5 (0.2) | <0.19 | 0.41 (0.12) |
| V821 Her | 7.7 (0.4) | 0.29 (0.16) | 1.33 (0.22) |
| RV Aqr | 2.2 (0.2) | <0.13 | 0.39 (0.14) |
| S Stars | |||
| R And | 0.83 (0.29) | <0.16 | <0.3 |
| S Cas | 1.3 (0.2) | <0.18 | <0.2 |
| R Gem | 0.34 (0.26) | <0.23 | <0.3 |
| RS Cnc | 1.0 (0.3) | 0.90 (0.16) | <0.3 |
| R Cyg | 0.41 (0.21) | <0.16 | <0.2 |
| M Stars | |||
| KU And | 3.7 (0.2) | <0.16 | 0.55 (0.15) |
| V370 And | ... | 1.07 (0.22) | ... |
| AFGL 292 | 0.16 (0.10) | <0.23 | <0.1 |
| R Hor | ... | 0.41 (0.18) | ... |
| NV Aur | 7.9 (0.2) | <0.13 | 1.25 (0.12) |
| BX Cam | 2.9 (0.2) | 0.85 (0.22) | 0.40 (0.11) |
| GX Mon | 6.2 (0.2) | <0.18 | 1.04 (0.12) |
| L2 Pup | ... | 1.13 (0.19) | ... |
| R LMi | ... | 0.54 (0.22) | ... |
| R Leo | ... | 1.46 (0.18) | ... |
| R Crt | ... | 1.73 (0.17) | ... |
| BK Vir | 0.04 (0.13) | 0.29 (0.17) | <0.1 |
| Y UMa | ... | 0.10 (0.18) | ... |
| RT Vir | ... | 0.87 (0.18) | ... |
| SW Vir | ... | 1.50 (0.22) | ... |
| R Hya | ... | 0.72 (0.18) | ... |
| RX Boo | ... | 1.63 (0.20) | ... |
| X Her | ... | 0.79 (0.27) | ... |
| V1111 Oph | 5.6 (0.3) | <0.19 | <0.3 |
| V1943 Sgr | ... | 0.37 (0.17) | ... |
| V1300 Aql | 11.0 (0.4) | <0.15 | 1.53 (0.22) |
| T Cep | ... | 0.32 (0.17) | ... |
| EP Aqr | ... | 2.00 (0.21) | ... |
Notes. The value in brackets after the flux gives the integrated noise rms. An ellipsis (...) indicates that the line was not observed for the indicated star. * indicates that flux has been corrected for ISM emission.
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