Table 1: Results of parametric calculations.
# $n_{\rm H,LIC}$ $n_{\rm p,LIC}$ R(TS) $F_{\rm H,TS}$a $F_{\rm O,TS}$ $F_{\rm N,TS}$
  cm-3 cm-3 AU      
1 0.16 0.032 109 0.58 0.72 (0.84) 0.80 (0.90)
2 0.16 0.05 102 0.55 0.70 (0.83) 0.80 (0.90)
3 0.16 0.06 99 0.54 0.70 (0.82) 0.80 (0.90)
4 0.16 0.07 96 0.53 0.69 (0.81) 0.80 (0.90)
5 0.18 0.032 101 0.57 0.69 (0.82) 0.77 (0.90)
6 0.18 0.05 96 0.54 0.68 (0.81) 0.79 (0.89)
7 0.18 0.06 93 0.53 0.68 (0.81) 0.79 (0.89)
8 0.18 0.07 88 0.52 0.66 (0.80) 0.79 (0.89)
9 0.20 0.032 94 0.55 0.68 (0.82) 0.76 (0.89)
10 0.20 0.04 93 0.54 0.67 (0.81) 0.77 (0.89)
11 0.20 0.05 90 0.53 0.67 (0.79) 0.78 (0.89)
12 0.20 0.06 88 0.52 0.67 (0.80) 0.78 (0.89)
13 0.20 0.07 86 0.51 0.67 (0.79) 0.78 (0.88)
a $F_ {A,\rm TS} = n_{A,\rm TS}/n_{A,\rm LIC}$ ($A={\rm H}$, O, N) are the filtration factors
  of interstellar H, O, N atoms, respectively.

Source LaTeX | All tables | In the text