RR Lyrae Stars and Anomalous Cepheids as Population Tracers in Local Group Galaxies

We discuss the use and importance of pulsating variable stars as population tracers in Local Group galaxies. Among bright variable crossing the classical instability strip, we mostly focus on RR Lyrae stars and Anomalous Cepheids. We discuss their pulsational properties and how it is possible to use them to constrain the evolution and star formation history of the host galaxy. We discuss RR Lyrae stars as tracers of the old population, and how they can be used to trace the accretion history of large galaxies such as the Milky Way and M31, and also the early chemical evolution. Moreover, we show that the frequency of Anomalous Cepheids follows different relations, and therefore trace the intermediate-age star formation. Finally, we discuss the different methods to derive distances and the impact of the Gaia mission.

Automated summary

This article discusses the use and importance of pulsating variable stars as population tracers in the Local Group galaxies. It focuses on RR Lyrae stars and Anomalous Cepheids, exploring their pulsational properties and how they can be utilized to understand the evolution and star formation history of host galaxies.