Dynamical effects of the radiative stellar feedback on the H I-to-H2 transition

Open Access

Fig. 3

N₁ integrated over the atomic region (dashed line), N₁ integrated over the molecular region (dotted line), N_1,tot (solid line) as functions of G₀∕n_H for a static and stationary approach. Black lines are for Eq. (9) of H₂ self-shielding, and red lines are for Eq. (5), both from Draine & Bertoldi (1996).

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