Table A.2
Integrated () line intensities in
K km s-1 for the HCN (v = 0,
J → J − 1) line emission used in the
excitation analysis.
Source | NRAO | OSO | SEST | JCMT | HHT | APEX | IRAM | ||||||||||||||
1 → 0 | 3 → 2 | 1 → 0 | 1 → 0 | 3 → 2 | 4 → 3 | 3 → 2 | 4 → 3 | 3 → 2 | 4 → 3 | 3 → 2 | 4 → 3 | 1 → 0 | 3 → 2 | ||||||||
|
|||||||||||||||||||||
M-type stars | |||||||||||||||||||||
RR Aql | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 0.41 | ··· | ··· | |||||||
RX Boo | ··· | ··· | 0.55 | ··· | ··· | ··· | 4.91 | 6.01 | 1.83 | 4.43 | ··· | ··· | 0.86 | ··· | |||||||
BX Cam | ··· | ··· | 1.35 | ··· | ··· | ··· | ··· | ··· | 2.33 | 3.73 | ··· | ··· | ··· | ··· | |||||||
TX Cam | ··· | ··· | 4.85 | ··· | ··· | ··· | 20.11 | 16.81 | 7.03 | 9.53 | ··· | ··· | 11.36 | 53.01 | |||||||
R Cas | ··· | ··· | 1.35 | ··· | ··· | ··· | 7.81 | 9.01 | 4.53 | 10.23 | ··· | ··· | 2.26 | ··· | |||||||
R Crt | ··· | ··· | ··· | 0.55 | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 3.31 | ··· | ··· | |||||||
R Dor | ··· | ··· | ··· | 0.65 | ··· | ··· | ··· | ··· | ··· | ··· | 7.71 | 8.11 | ··· | ··· | |||||||
R Hor | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 0.41 | ··· | ··· | |||||||
R Hya | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 1.31 | ··· | ··· | |||||||
W Hya | ··· | ··· | ··· | 0.45 | ··· | ··· | ··· | 10.81 | 6.83 | 10.73 | ··· | 3.11 | ··· | ··· | |||||||
R Leo | ··· | ··· | 0.45 | ··· | ··· | ··· | 5.51 | 6.91 | 1.83 | ··· | ··· | ··· | ··· | ··· | |||||||
AP Lyn | ··· | ··· | 1.25 | ··· | ··· | ··· | ··· | ··· | 1.73 | ··· | ··· | ··· | ··· | ··· | |||||||
GX Mon | ··· | ··· | 2.35 | ··· | ··· | ··· | ··· | ··· | ··· | 5.13 | ··· | ··· | ··· | ··· | |||||||
WX Psc | ··· | ··· | 3.75 | ··· | ··· | ··· | 9.01 | ··· | 5.03 | ··· | ··· | ··· | ··· | ··· | |||||||
L2 Pup | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 1.11 | ··· | ··· | |||||||
IK Tau | ··· | ··· | 3.55 | ··· | ··· | ··· | 23.61 | 35.21 | ··· | ··· | ··· | ··· | 11.26 | ··· | |||||||
RT Vir | ··· | ··· | 0.35 | ··· | ··· | ··· | 1.61 | ··· | ··· | ··· | ··· | ··· | ··· | ··· | |||||||
SW Vir | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 0.83 | 1.73 | ··· | 1.31 | ··· | ··· | |||||||
CIT 4 | ··· | ··· | 0.75 | ··· | ··· | ··· | 2.31 | ··· | ··· | ··· | ··· | ··· | ··· | ··· | |||||||
IRC-10529 | ··· | ··· | 1.05 | ··· | ··· | ··· | ··· | ··· | 1.93 | 3.93 | ··· | 2.21 | 2.06 | ··· | |||||||
IRC-20197 | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 1.11 | ··· | ··· | |||||||
IRC-30398 | ··· | ··· | ··· | 0.45 | ··· | ··· | ··· | ··· | 1.33 | 2.03 | ··· | 2.71 | ··· | ··· | |||||||
IRC+10365 | ··· | ··· | 2.05 | ··· | ··· | ··· | ··· | ··· | 2.13 | 4.23 | ··· | ··· | ··· | ··· | |||||||
IRC+40004 | ··· | ··· | ··· | ··· | ··· | ··· | ··· | ··· | 1.83 | 4.73 | ··· | ··· | ··· | ··· | |||||||
IRC+50137 | ··· | ··· | 0.95 | ··· | ··· | ··· | 3.61 | ··· | ··· | ··· | ··· | ··· | ··· | ··· |
Notes.
Bieging et al. (2000). Data from the Arizona Radio Observatory Submillimeter Telescope (ARO SMT), previously known as the Heinrich Hertz Submillimeter Telescope (HHT).
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