Description
This article will study stellar parameters, based on equations and notions of theoretical physics, demonstrating how it is possible to obtain and understand the Lane-Emden equation, analyzing some aspects in a didactic way.
A Python computational language was used, attached to a numerical resolution method known as Runge-Kutta, with these tools it was possible to build some graphics and a data table, which relates the stellar parameters with the indexed numbers of the theoretical model.
Primary author
Marcos Vinicius Bernardes
(Unifal-Universidade Federal de Alfenas)
