All Tables

• Table 1: IRAS 16293-2422 physical structure from dust modeling by Schöier et al. (2002).
• Table 2: Initial abundances at t=0 relative to H₂ for AFGL 2591.
• Table 3: Differences between best fit model for IRAS 16293-2422 and AFGL 2591.
• Table 4: IRAS 16293-2422 predicted column densities (cm^-2).