Table A.4: "Distance-independent'' parameters of the clumps. The angular diameters, $\theta $, and integrated flux densities, $F_{\nu }$, have been derived from the 1.2 mm continuum maps; the rotation temperatures, $T_{\rm rot}$, the C17O column densities, $N_{\rm C^{17}O}$, and the H2 total column densities, $N_{\rm H_{2}}$, have been derived from C17O line ratios (assuming a C17O mean abundance of 3.9 $\times $ 10-8); the ${\rm H}_{2}$ volume densities, $n_{\rm H_2}$, have been obtained from CS line ratios.
Source $\theta $ $F_{\nu }$ $T_{\rm k}$ $N_{\rm C^{17}O}$ $N_{\rm H_{2}}$ $n_{\rm H_2}$
  ( $^{\prime \prime }$) (Jy) (K) ( $\times10^{15}$cm-2) (cm-2) (cm-3)
08211-4158 34.3 2.26 12 2.3 5.9 $\times $ 1022 1.2 $\times $ 105
08563-4225 29.5 4.09 10 7.6 1.9 $\times $ 1023 1.7 $\times $ 105
09014-4736 42.1 0.79        
09026-4842 65.8 1.25 15 1.0 2.5 $\times $ 1022 6.3 $\times $ 105
09131-4723 71.6 4.5 14 1.7 4.3 $\times $ 1022 4.2 $\times $ 105
09166-4813     11 0.4 1.1 $10\times^{22}$  
09209-5143 64.5 1.43        
10095-5843 33.9 1.16 9 1.8 4.7 $\times $ 1022 1.5 $\times $ 105
10123-5727 43.2 2.41       1.7 $\times $ 105
10277-5730 27.0 0.63       4.9 $\times $ 104
10308-6122 33.8 0.45       2.1 $\times $ 105
10439-5941 42.8 6.90        
10521-6031 6.5 0.46        
10548-5929 65.5 0.62       5.2 $\times $ 104
10554-6237 21.5 0.73 8 2.9 7.4 $\times $ 1022 4.0 $\times $ 104
10572-6018 37.5 1.31       4.2 $\times $ 104
11265-6158 30.3 0.50       2.1 $\times $ 105
11294-6257 17.9 0.27        
11380-6311 51.1 2.53       1.8 $\times $ 105
11404-6215 9.5 0.70        
12295-6224 45.9 2.4 11 1.6 4.2 $\times $ 1022 1.4 $\times $ 105
12377-6237 15.1 0.53        
13023-6213 28.5 1.39        
13039-6108 50.9 1.38 18 0.7 1.9 $\times $ 1022 1.7 $\times $ 105
13106-6050 33.5 1.95 8 4.5 1.1 $\times $ 1023 5.7 $\times $ 104
13333-6234 31.8 1.5 8 3.7 9.4 $\times $ 1022 2.2 $\times $ 105
13384-6152 30.0 0.45 9 4.2 1.1 $\times $ 1023  
13395-6153 24.5 4.2 10 6.8 1.7 $\times $ 1023 8.9 $\times $ 104
13438-6203 33.4 3.9 6 1.8 4.7 $\times $ 1022  
13481-6124 25.5 7.12 18 2.8 7.1 $\times $ 1022 1.2 $\times $ 105
13560-6133 18.5 3.1 7 6.0 1.6 $\times $ 1023 1.5 $\times $ 105
14000-6104 50.5 4.4 11 1.3 3.3 $\times $ 1022 4.2 $\times $ 105
14131-6126 $\ll$21 ($^{\char93 }$) 0.27 6 43.0 1.1 $\times $ 1024 1.7 $\times $ 105
14166-6118 48.9 1.06 8 2.4 6.1 $\times $ 1022 7.1 $\times $ 104
14183-6050 38.4 0.35       1.7 $\times $ 105
14201-6044     23 1.3 3.4 $\times $ 1022  
14395-5941 $\ll 21$ ($^{\char93 }$) 0.46 6 46.1 1.2 $\times $ 1024 2.8 $\times $ 104
14425-6023 20.7 1.46 8 7.4 1.9 $\times $ 1023  
15038-5828     17 0.6 1.6 $\times $ 1022  
15072-5855 23.6 1.02 8 4.8 1.2 $\times $ 1023 1.2 $\times $ 105
15100-5903 28. 0.95 5 2.4 6.2 $\times $ 1022 2.8 $\times $ 104
15219-5658 15.2 0.52       5.3104
15246-5612 20.2 1.26 7 8.4 2.2 $\times $ 1023 4.5 $\times $ 104
15262-5541 46.9 1.82 10 0.5 1.3 $\times $ 1022  
15347-5518 48.4 3.12 8 2.1 5.3 $\times $ 1022 2.2 $\times $ 105
15371-5458 43.3 0.67       3.5 $\times $ 105
15470-5419 39.5 2.41 7 3.1 8.0 $\times $ 1022 2.0 $\times $ 105
15519-5430 32.1 6.38 12 6.4 1.6 $\times $ 1023 2.8 $\times $ 105
15557-5337 38.9 16.7 18 10.3 2.6 $\times $ 1023 3.7 $\times $ 104
15579-5303 21.3 6.26 6 9.2 2.4 $\times $ 1023  
15583-5314 39.3 0.53 10 2.7 6.9 $\times $ 1022 1.3 $\times $ 105
16061-5048 27.7 1.64 6 4.8 1.2 $\times $ 1023  
16082-5031 35.1 0.54 7 3.6 9.2 $\times $ 1022  
16093-5015 34.8 1.81 8 2.9 7.5 $\times $ 1022 8.4 $\times $ 104
16093-5128 43.0 1.28 8 2.1 5.5 $\times $ 1022  
16106-5048     11 0.8 2.0 $\times $ 1022  
16107-4956     6 0.4 1.1 $\times $ 1022  
16148-5011 12.4 2.32 8 11.6 3.0 $\times $ 1023  
16187-4932 35.2 0.66        
16194-4934     7 1.3 3.3 $\times $ 1022  
16204-4916 32.0 1.37 8 2.2 5.7 $\times $ 1022 2.4 $\times $ 104
16218-4931 16.4 0.69 6 10.1 2.6 $\times $ 1023 2.6 $\times $ 104
16232-4917 16.6 0.45       4.5 $\times $ 104
16252-4853 43.1 1.22 6 1.2 3.2 $\times $ 1022 2.4 $\times $ 104
16254-4844     12 1.1 2.9 $\times $ 1022  
16344-4605 26.6 2.85 7 4.7 1.2 $\times $ 1023  
16363-4645 13.0 0.22       5.7 $\times $ 104
16369-4810     8 1.8 4.7 $\times $ 1022  
16403-4614     8 0.5 1.3 $\times $ 1022  
16419-4602 17. 2.27 9 2.1 5.3 $\times $ 1022  
16464-4359 42. 1.4 10 2.3 5.9 $\times $ 1022 7.1 $\times $ 104
16501-4314 70.9 2.15 15 1.7 4.3 $\times $ 1022 1.0 $\times $ 105
16535-4300 42.0 0.87 8 2.5 6.5 $\times $ 1022 3.5 $\times $ 104
17033-4035     15 1.5 3.7 $\times $ 1022  
17036-4033     10 0.7 1.9 $\times $ 1022  
17040-3959 15.6 0.95 7 8.5 2.2 $\times $ 1023 2.4 $\times $ 104
17082-4114 50. 7.13 8 3.1 7.9 $\times $ 1022  
17156-3607     10 0.8 2.0 $\times $ 1022  
17211-3537 36.8 1.1 7 1.6 4.2 $\times $ 1022 5.5 $\times $ 104
17218-3704 45.4 1.44 9 1.7 4.3 $\times $ 1022 1.7 $\times $ 105
17225-3426     10 1.7 4.3 $\times $ 1022  
17230-3531 21.6 1.19 7 10.9 2.8 $\times $ 1023 4.2 $\times $ 104
17256-3631 18.7 5.6 45 2.0 5.2 $\times $ 1022 7.1 $\times $ 104
17285-3346 11.9 0.26        
17338-3044 19.0 0.19        
17355-3241 45.5 0.6 8 2.2 5.7 $\times $ 1022 4.2 $\times $ 104
17377-3109 17.5 2.0 6 22.7 5.812 $\times $ 1023 1.1 $\times $ 105
17410-3019 18.7 0.16 7 8.2 2.1 $\times $ 1023  
17425-3017 21.1 1.59 7 5.1 1.3 $\times $ 1023 2.7 $\times $ 104

$^{\char93 }$ Unresolved sources.


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations
3 Observational results
4 Derivation of the physical parameters
5 Discussion
6 Conclusions
References
Online Material
List of tables
List of figures