Morphology of the nova ejecta

In this work, we aim to analyze the morphology of the ejected material from a nova explosion. During this experiment, YT and Python coding were used to read the data of a simulated star explosion. This is then used to evaluate various aspects of the ejected material, such as chemical compounds, temperatures, and density. Our findings indicate that these quantities present nonuniform distributions, possibly due to the behavior of turbulence during the nova explosion.