Double riches: asteroseismology in eclipsing binaries
John Southworth (Keele University, UK)
TL;DR
This paper discusses combining asteroseismology with eclipsing binary analysis to improve stellar property measurements and test stellar evolution models.
Contribution
It reviews recent progress and proposes future directions for integrating asteroseismology with eclipsing binary studies.
Findings
Enhanced accuracy in stellar property determination
Improved calibration of asteroseismic models
Potential for stringent tests of stellar evolution theories
Abstract
The study of eclipsing binaries is our primary source of measured properties of normal stars, achieved through analysis of light and radial velocity curves of eclipsing systems. The study of oscillations and pulsations is increasingly vital for determining the properties of single stars, and investigating the physical phenomena active in their interiors. Combining the two methods holds the promise of establishing stringent tests of stellar evolutionary theory, and of calibrating model-dependent asteroseismology with empirically measured stellar properties. I review recent advances and outline future work.
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