The space photometry revolution and our understanding of RR Lyrae stars

TL;DR

Recent space-based photometry has unveiled complex pulsation behaviors in RR Lyrae stars, revealing intricate mode interactions and offering new insights into the longstanding Blazhko phenomenon.

Contribution

This paper provides an overview of new observational and theoretical findings on RR Lyrae stars, highlighting the role of multi-mode interactions and complex dynamics in their variability.

Findings

Detection of period doubling and Blazhko modulation connection

Presence of additional periodicities in RR Lyrae subtypes

Complex dynamical states from multi-mode interactions

Abstract

The study of RR Lyrae stars has recently been invigorated thanks to the long, uninterrupted, ultra-precise time series data provided by the Kepler and CoRoT space telescopes. We give a brief overview of the new observational findings concentrating on the connection between period doubling and the Blazhko modulation, and the omnipresence of additional periodicities in all RR Lyrae subtypes, except for non-modulated RRab stars. Recent theoretical results demonstrate that if more than two modes are present in a nonlinear dynamical system such as a high-amplitude RR Lyrae star, the outcome is often an extremely intricate dynamical state. Thus, based on these discoveries, an underlying picture of complex dynamical interactions between modes is emerging which sheds new light on the century-old Blazhko-phenomenon, as well. New directions of theoretical efforts, like multi-dimensional hydrodynamical simulations, future space photometric missions and detailed spectroscopic investigations will pave the way towards a more complete understanding of the atmospheric and pulsation dynamics of these enigmatic touchstone objects.