Image Details
Caption: Figure 4.
Demonstrating the sensitivity of each parameter on the CO fundamental band of Model P at day 385 (see Table 1), where the temperature profile has been optimized for each. Panel (A) shows the best-fit solution and continuum. Each of the following panels keeps the optimized parameters the same but shows the effect of: (B) the total molecular mass (M), (C) the inner temperature (T1), (D) the density structure (n), (E) the inner velocity edge (v1), (F) the width of the molecular region (Δv), (G) the clump density contrast (fc), (H) the clump size (rR), and (I) the clump shape (ϵ). Figures 6 and 7 show the ﹩{\chi }_{* }^{2}﹩ convergences of the fits.
© 2026. The Author(s). Published by the American Astronomical Society.