Study of physical properties of main – Sequence stars
Study of physical properties of main – Sequence stars
In astrophysics, we can study physical properties of stars by analyzing their spectra and building theoretical models of stellar structure. In this report Study of physical properties of main – Sequence stars, we have used the CLEA program to classify stellar spectra and determine the physical properties of a number of main-sequence stars. Furthermore, we have used a numerical algorithm and a FORTRAN program to study theoretical models of stellar structure.