Table 4
RMS noise for all observed H2S lines from APEX survey.
H2S | H234S | |||
Star | 11,0 → 10,1 | 22,0 → 21,1 | 33,0 → 32,1 | 11,0 → 10,1 |
|
||||
M-type stars | ||||
R Hor | 11 | ... | 13 | 11 |
IK Tau | 18D | 17T | 20 | 18 |
GX Mon | 20D | 12 | 18 | 20 |
W Hya | 16 | ... | 11 | 16 |
RR Aql | 19 | 15 | 13 | 19 |
V1943 Sgr | 13 | ... | 11 | 13 |
V1300 Aql | 13D | 20 | 15T | 13T |
V1111 Oph | 13D | ... | ... | 13 |
WX Psc | 8D | ... | ... | 8D |
IRC-30398 | 13 | ... | ... | 13 |
|
||||
S-type stars | ||||
T Cet | ... | 13 | ... | ... |
TT Cen | 20 | ... | 10 | 20 |
W Aql | 13 | 14 | 14 | 13 |
RZ Sgr | 20 | ... | 13 | 20 |
|
||||
Carbon stars | ||||
R Lep | ... | 16 | ... | ... |
V1259 Ori | 17 | 14 | 15 | 17 |
AI Vol | 20 | 17 | ... | 20 |
X TrA | ... | 13 | ... | ... |
II Lup | 10* | 11 | 10 | ... |
V821 Her | 19 | 18 | ... | 19 |
RV Aqr | ... | 15 | ... | ... |
Notes. RMS values given in mK at a velocity resolution of 1 km s-1. (...) indicates lines that were not observed, (D) and (T) indicate detected or tentatively detected lines, respectively (see Table 3 for integrated intensities). (*) indicates that the APEX observation is from De Beck et al. (in prep.).
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