Table B.3
HIFI and IRAM CN and H3CN line group observations.
| Star | CN | HC3N | ||||||
| 11/2 → 01/2 | 13/2 → 01/2 | 23/2 → 11/2 | 23/2 → 13/2 | 25/2 → 13/2 | 59/2 → 47/2 | 511/2 → 49/2 | 12 → 11 | |
| [K km s-1] | [K km s-1] | [K km s-1] | [K km s-1] | [K km s-1] | [K km s-1] | [K km s-1] | [K km s-1] | |
|
|
||||||||
| R Scl | 15.6 (1.0) | 13.2 (1.0) | 31.4 (0.9) | 7.1 (0.9) | 25.2 (0.9) | 3.0 (0.1) | 1.7 (0.1) | <1.0 |
| V701 Cas | 3.7 (0.3) | 8.5 (0.3) | 5.0 (0.4) | <0.4 | 6.3 (0.4) | <0.2 | <0.2 | 1.76 (0.17) |
| V384 Per | 21.6 (0.2) | 28.4 (0.2) | 21.9 (0.3) | 7.0 (0.3) | 23.3 (0.3) | <0.2 | <0.2 | 3.72 (0.12) |
| GY Cam | 13.8 (0.2) | 10.9 (0.2) | 16.2 (0.3) | 3.7 (0.3) | 12.9 (0.3) | <0.2 | <0.2 | 0.69 (0.17) |
| R Lep | 11.8 (0.4) | 11.7 (0.4) | 37.2 (0.6) | 6.8 (0.6) | 29.5 (0.6) | 2.0 (0.1) | 1.2 (0.1) | <0.4 |
| V1259 Ori | 6.1 (0.2) | 12.6 (0.2) | 4.6 (0.3) | <0.3 | 8.9 (0.3) | <0.2 | <0.2 | 3.13 (0.16) |
| V688 Mon | 4.2 (0.3) | 8.7 (0.3) | 8.1 (0.2) | <0.2 | 11.6 (0.2) | <0.2 | <0.2 | 2.40 (0.15) |
| U Hya | <0.4 | 1.4 (0.4) | 17.1 (1.0) | <1.0 | 11.6 (1.0) | 1.8 (0.2) | 1.1 (0.2) | <0.4 |
| X TrA | ... | ... | ... | ... | ... | 1.0 (0.2) | 0.7 (0.2) | ... |
| V821 Her | 15.8 (0.5) | 22.6 (0.5) | 17.1 (0.7) | <0.7 | 25.2 (0.7) | <0.2 | <0.2 | 2.26 (0.24) |
| V Aql | 4.4 (0.2) | 4.9 (0.2) | 10.6 (0.3) | 2.4 (0.3) | 13.0 (0.3) | <0.1 | <0.1 | 0.26 (0.08) |
| V1968 Cyg | 3.0 (0.3) | 5.6 (0.3) | ... | ... | ... | <0.2 | <0.2 | 1.06 (0.14) |
| RV Aqr | 14.7 (0.2) | 15.7 (0.2) | 22.2 (0.4) | 4.7 (0.4) | 20.2 (0.4) | <0.1 | <0.1 | 0.28 (0.15) |
| S Cas | <0.3 | 1.4 (0.3) | 11.8 (0.5) | 2.4 (0.5) | 11.6 (0.5) | <0.2 | <0.2 | <0.3 |
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. An * indicates the line was detected but contaminated by an artefact and the integrated intensity cannot be relied upon.
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