Table 5
H2O peak flux density (first entry in mJy) and velocity extent (second entry in km s−1, highlighted with italics) of observed lines for an aperture diameter of 0.′′08 extracted from the extended configuration.
| Star | Line 1 | Line 4 | Line 5 | Line 6 | Line 7 | Line 8 | Line 10 | Line 12 | Line 13 | Line 14 |
|---|---|---|---|---|---|---|---|---|---|---|
| 222.014 | 236.805 | 244.330 | 252.172 | 254.040 | 254.053 | 259.952 | 262.898 | 266.574 | 268.149 | |
| S Pav | 15 | – | −10(a) | 18 | 9 | 7 | 28 | 31 | 18 | 173 |
| 10.5 | 11.3 | 11.6 | ? (c) | ? (c) | 12.4 | 13.4 | 6.6 | 19.7 | ||
| T Mic | – | – | – | 15 | 10 | abso.?(d) | 16 | 21 | 11 | 99 |
| 10.4 | 8.6 | 79 | 8.9 | 5.5 | 22.9 | |||||
| U Del | – | – | – | – | – | – | – | – | – | 5 |
| 14.5 | ||||||||||
| RW Sco | – | – | – | – | – | – | – | 25 | – | 93 |
| 5.6 | 10.9 | |||||||||
| V PsA | – | – | – | – | – | – | – | 14 | – | 23 |
| 8.9 | 16.4 | |||||||||
| SV Aqr | – | – | – | – | – | – | – | – | – | 10 |
| 5.5 | ||||||||||
| R Hya | 16 | 5? | −8(c) | 20 | 14 | 10 | 29 | 38 | 23 | 119 |
| 10.5 | 13.0? | 12.0 | 16.3 | 12.7 | 8.1(c) | 15.8 | 15.6 | 12.1 | 22.9 | |
| U Her | 10 | – | – | 10 | 12 | – | 16 | 36 | – | 209 |
| 6.6? | 7.0 | 6.3 | 11.3 | 15.6 | 18.6 | |||||
| AH Sco | 8 | – | – | 6 | 10 | – | 33 | 20 | 9 | 68974 |
| 7.9 | 4.8 | 5.8 | 5.6 | 5.6 | 5.5 | 29(e) | ||||
| R Aql | 10 | – | −7.5(a) | 22 | 10 | 7 | 18 | 43 | 21 | 220 |
| 14.3 | 6.5 | 11.6 | ?(c) | 17.7 | 12.3 | 8.8 | 8.6 | |||
| GY Aql | – | – | – | – | – | – | 25 | 35 | – | 159 |
| 7.1 | 7.8 | 13.1 | ||||||||
| KW Sgr | – | – | – | – | – | – | – | – | – | 10 |
| 8.5 | ||||||||||
| IRC–10529 | 14 | – | – | – | 31 | 17 | 39 | 45 | – | 92 |
| 6.2 | 5.8 | ? | 9.0 | 6.7 | 6.5 | |||||
| IRC+10011 | 37 | – | abso.(b) | 19 | 49 | 13 | 86 | 100 | 43 | 1823 |
| 6.6 | 6.9 | 10.4 | 7.6 | 10.1 | 11.1 | 9.9 | 15.3 | |||
| VX Sgr | 8 | – | – | 14 | 11 | – | 27 | 49 | 20 | 440 |
| 6.6 | 7.0 | 5.8 | 13.7 | 17.8 | 6.6 | 25(e) |
Notes. The approximate frequency is given in GHz below each line number (quantum numbers and exact frequency given in Table 2). Typical peak flux density uncertainties are 1–4 mJy. The velocity range is defined as the difference between the red and blue velocities for line emission above 2.5σ. A question mark indicates an uncertain value. No detection is indicated with –.(a) Absorption line profiles and maps in Figs. 5 and 8. (b)Uncertain line parameters; zeroth moment map shows unresolved 3σ absorption with the combined array (Fig. 8). (c)Uncertain velocity extent due to absorption on redshifted side of emission line.(d) Apparent redshifted absorption in extended and combined configuration data without emission. (e)Estimate of the 268.149 GHz velocity extent hindered by a nearby broad SO2 feature.
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