Same as Fig. 8 but for four different GMCs. The top row has models that has no drag and does not consider latent heat release from dissociation and recombination of H₂ (Parmentier et al. 2018). The next three rows are maps of models that consider the dissociation and recombination of H₂ (Tan et al. 2024). The difference comes in the drag timescale: τ_drag = ∞ (no drag), τ_drag = 10⁶ s (weak drag), and τ_drag = 10⁴ s (strong drag). The left column maps consider both pre- and post-eclipse phases. The middle column includes the maps when considering only the pre-eclipse phases. In the right column are the maps of the post-eclipse phases only.