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Table 2

Parameters used in the shell model and resulting mean temperature and density of hydrogen.

Source Integration Integration limits (radii) Emission(b) (H2)(c) (H2)(d) H2

rstart/Tup rend/Tlow region particle
settings(a) (model) number(e)
[AU]/[K] [AU]/[K] [′′] [K] [cm−3] [#]
R CrA-IRS 5A A 72/100 10 000/10 153.′′8 12.7 6.1 × 104 8.5 × 1056
B 683/35 4 194/15 64.′′5 18.6 1.2 × 105 1.2 × 1056
NGC 1333-IRAS 2A A 207/100 17 000/10 144.′′7 16.2 3.2 × 104 2.2 × 1057
B 1546/35 7823/15 66.′′6 20.5 1.1 × 105 7.0 × 1056
L1551-IRS 5 A 168/100 14 000/10 200.′′0 16.9 2.6 × 104 9.9 × 1056
B 1265/35 6425/15 91.′′8 20.7 9.1 × 104 3.4 × 1056
L1544 C 1/12.5 8000/12.5 114.′′3 12.5 1.3 × 106 (f) 9.1 × 1057

Notes. (a) Two integration settings have been used (A, B) starting at rstart and ending at rend depending on the temperature region to be covered (A = 10–100 K, and B = 15–35 K), C indicates a flat density and temperature distribution of hydrogen. (b) Outer diameter of region where our investigated molecules, e.g., H2CO or CH3OH, emit radiation according to our model. (c)Hydrogen mean temperature. (d)Hydrogen mean particle density. (e)Absolute number of hydrogen particles within integration limits. This number is used to calculate the values in Tables 3 and 4. (f)Value from Caselli et al. (2002) for inner 40′′ region.

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