"In this Bachelor’s Degree Thesis, we will first work towards the derivation of the equations of stellar structure and evolution, and then we will dive into the most widely used algorithm to solve them: The Henyey method. After that, we will generate and evolve some solar models and study in detail some of their structural properties. To achieve this we will make use of AMUSE- the Astrophysical Multipurpose Software Environment developed by Simon Portegies Zwart and Steve McMillan."
This repository contains all the files for this project. You will find the IMPLEMENTATION AND REPRODUCIBILITY instructions here.