Table 1: Parameters adopted in the simulations.
Model $\xi_{\max}$ a $\rho_{\rm c}$ b M0 c Spectral type of d d
    [ ${\rm g ~ cm^{-3}}$] [$M_{\odot}$] ionizing star [pc]

A		 3 $1.05 \times 10^{-20}$ 3 O8V 3-10
B 4 $3.01 \times 10^{-20}$ 3 O8V 3-10
C 5 $6.09 \times 10^{-20}$ 3 O8V 3-10
D 3 $1.05 \times 10^{-20}$ 3 O4V 3-10
E 4 $3.01 \times 10^{-20}$ 3 O4V 3-10
F 5 $6.09 \times 10^{-20}$ 3 O4V 3-10
G 5 $6.09 \times 10^{-22}$ 30 O8V 3-10
a Non-dimensional truncation radius of initial core (Bonnor-Ebert sphere).
b Central density of initial core.
c Total mass of initial core.
d Distance from ionizing star.

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