Astrophysical flows transport mass, momentum, and energy, shape to their surrounding environments, and contribute to the physical and chemical evolution of the interstellar medium. Understanding their dynamics, morphology, and chemical signatures requires combining theoretical models with multiwavelength observations. In this talk, I will highlight my main scientific contributions to the modeling of astrophysical flows, focusing primarily on protostellar outflows across different physical regimes. I will present the development and application of the chemo-hydrodynamical code WALKIMYA-2D to model the dynamics and chemical evolution of the Cep E outflow, as well as my contributions to the analytical modeling of the outflow in L1551 IRS 5. I will also discuss my work on the origin and physical mechanisms behind the complex kinematics and morphology of explosive outflows. These studies illustrate my approach of combining numerical and analytical models with molecular observations to investigate mass-ejection processes and their impact on the surrounding environment. Building on this experience, I will describe my current research, which combines theoretical modeling with molecular interferometric observations to investigate the dynamics, interactions, and chemical evolution of astrophysical flows. Finally, I will present my future research plans, focusing on outflow interactions and collisions in multiple stellar systems, their contribution to the chemical enrichment of star-forming regions, and the extension of chemo- dynamical modeling approaches to other astrophysical environments, including evolved stars and galactic winds. These efforts aim to establish a broader framework for understanding the role of astrophysical flows in the evolution of astronomical systems.