A Grid of Core Collapse Supernova Remnant Models Evolved from Massive Progenitors

We present preliminary results from modeling core-collapse supernovae evolved from pre-main sequence models with wind-driven mass loss. We construct a software pipeline to follow the massive star evolution beginning with modelling up to iron core collapse with MESA. We then use the Supernova Evolution Code (SNEC) to explode the star and follow the evolution of the ejecta with the cosmic ray hydro (ChN) code. ChN allows us to model the remnant's dynamics and broadband spectrum as a function of age. We quantify the impact of progenitor evolution on the bulk observable characteristics of the remnant, including its dynamics and spectral properties.