RR Lyrae and Type II Cepheid Variables in Globular Clusters: Optical and Infrared Properties

TL;DR

This paper reviews the properties, evolutionary stages, and period-luminosity relations of RR Lyrae and type II Cepheid variables in globular clusters, emphasizing their role as standard candles for distance measurement.

Contribution

It provides a comprehensive analysis of pulsation properties and multiband period-luminosity-metallicity relations for these variables in globular clusters.

Findings

Detailed period-luminosity relations across optical and infrared wavelengths.

Calibration of the RR Lyrae visual magnitude-metallicity relation.

Insights into the evolutionary stages of pulsating variables.

Abstract

Globular clusters are both primary fossils of galactic evolution and formation and are ideal laboratories for constraining the evolution of low-mass and metal-poor stars. RR Lyrae and type II Cepheid variables are low-mass, radially pulsating stars that trace old-age stellar populations. These stellar standard candles in globular clusters are crucial for measuring their precise distances and, in turn, absolute ages, and for the calibration of the extragalactic distance scale. Herein, the evolutionary stages of RR Lyrae and type II Cepheids are discussed, and their pulsation properties, including the light curves, color-magnitude and period-amplitude diagrams, and period-luminosity relations in globular clusters at optical and infrared wavelengths are presented. The RR Lyrae visual magnitude-metallicity relation and the multiband period-luminosity-metallicity relations in globular clusters covering a wide metallicity range are also discussed in detail for their application to the RR Lyrae-based distance~scale.