Computational insights into the chemical reaction networks of C ₃ H ₆ O ₃ , C ₃ H ₇ O ₃ and C ₂ H ₅ O ₂ : implications for the interstellar medium

)-ethene-1,2-diol dominate many pathways and align better with current astronomical observations. This work provides detailed mechanistic and kinetic insights that enhance astrochemical modeling and advance our understanding of molecular complexity in star-forming environments. Furthermore, it highlights the utility of automated CRN exploration for uncovering viable synthetic routes to prebiotic molecules in space.