Table 2: Summary of single-dish millimetre line observations used in the analysis.
Source Telescope Transition $\int T_{{\rm mb}}{\rm d}v$ Ref.
      [K km s-1]  
R Scl IRAM CO(1-0) 76.2 4
  IRAM CO(2-1) 67.7 4
  SEST CO(1-0) 26.1 4
  SEST CO(2-1) 47.8 4
  SEST CO(3-2) 63.7 3
  JCMT CO(2-1) 50.6 6
  JCMT CO(3-2) 62.8 1
  JCMT CO(4-3) 63.2 1
  SEST 13CO(1-0) 1.9 5
  SEST 13CO(2-1) 4.2 5
  SEST HCN(1-0) 1.3 3
  SEST HCN(3-2) 7.7 3
  SEST HCN(4-3) 3.9 3
  HHT HCN(3-2) 2.4 7
  HHT HCN(4-3) 4.1 7
U Cam IRAM CO(1-0) 21.8 1
  IRAM CO(2-1) 97.9 1
  JCMT CO(3-2) 66.7 1
  JCMT CO(4-3) 54.6 1
U Ant SEST CO(1-0) 10.8 3
  SEST CO(2-1) 13.1 3
  SEST CO(3-2) 9.7 3
V644 Sco SEST CO(1-0) 7.6 3
  SEST CO(2-1) 20.7 3
  SEST CO(3-2) 21.4 3
  JCMT CO(2-1) 22.2 6
  JCMT 13CO(2-1) 1.1 1
  SEST HCN(1-0) 0.3 1
  SEST HCN(3-2) 0.4 1
DR Ser SEST CO(1-0) 3.7 2
  NRAO CO(2-1) 11.3 2
  JCMT CO(3-2) 14.7 1
  JCMT CO(4-3) 8.5 1
  OSO HCN(1-0) 0.6 1
S Sct SEST CO(1-0) 5.8 3
  SEST CO(2-1) 4.3 3
  SEST CO(3-2) 3.1 3
  SEST 13CO(1-0) 0.2 3
TT Cyg SEST CO(1-0) 5.0 1
  OSO CO(1-0) 6.4 3
  IRAM CO(1-0) 7.5 3
  IRAM CO(2-1) 6.0 3
Refs. - 1) This paper; 2) Schöier & Olofsson (2001); 3) Olofsson et al. (1996); 4) Olofsson et al. (1993b);
5) Schöier & Olofsson (2000); 6) JCMT public archive; 7) Bieging (2001).

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations
3 Radiative transfer
4 Dust modelling
5 Molecular line modelling
6 Discussion
7 Conclusions
References
List of tables
List of figures