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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. 

(1)

This paper.

(3)

Bieging et al. (2000). Data from the Arizona Radio Observatory Submillimeter Telescope (ARO SMT), previously known as the Heinrich Hertz Submillimeter Telescope (HHT).

(4)

JCMT public archive.

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