High Power Accretion in Massive Binary Systems and Impact of Metallicity

The dataset provided includes all the necessary files to run the MESA code for our numerical experiment on accretion mechanics in massive stars for three different mateallicities e.g., Glactic (Z=0.02), LMC (Z=0.008), and SMC (Z=0.008). Specifically, it contains the inlist file with all input parameters for the stellar modeling, as well as the rn and mk files required for MESA compilation. We also include the history and profile files, which store the data points used to generate plots like parameters: lumiosty, temapture, radius, mass, entropy, and enrgies. Additionally, we provide Python scripts used to create the graphs from the output data.