Variable Stars and Their Implications for Stellar Astrophysics

Abstract

The paper provides a review on the relationship between the variation of some stars with certain evolutionary features, with particular emphasis on how stellar pulsations and eruptions aid in the understanding of stellar evolution theories. It analyzes and discusses light curves, spectral classifications, and periodicity measurements of different variable stars to gain a better understanding of the processes that transfer energy and the mechanisms that cause pulsation. Results suggest that certain subclasses of variable stars, especially the Cepheid and the RR Lyrae variable stars, obey some certain trends of mass and luminosity which are very stringent bounds for the existing stellar evolution models. Furthermore, the new modes of pulsations described in this paper are capable of overturning the established paradigms of stellar astrophysics and may define new boundaries of astrophysical research. The paper also emphasizes the importance of the dynamics of stellar populations in the refinement of cosmological models related to the evolution of galaxies and the universe in general, which makes these models more realistic. This work makes a point on the strong correlation between the variability of stars and the profound questions in time, state of equilibrium, and change in the system that is being studied: the dynamics of natural systems.