TL;DR
This review discusses the current state and future prospects of stellar seismology in active stars, emphasizing how space-based photometry from missions like Kepler will enhance understanding of their internal structures and processes.
Contribution
It highlights the potential for significant advances in understanding active stars through upcoming space-based photometric data and discusses current open questions in stellar seismology.
Findings
Longer photometric timeseries enable better internal structure analysis.
Kepler data will significantly improve understanding of active star processes.
Open questions remain about star-activity interactions.
Abstract
In this review we will discuss the current standing and open questions of seismology in active stars. With the longer photometric timeseries data that are --and will become-- available from space-missions such as Kepler we foresee significant progress in our understanding of stellar internal structures and processes --including interactions between them-- taking place in active stars in the next few years.
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