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Double riches: asteroseismology in eclipsing binaries

Published online by Cambridge University Press:  27 October 2016

John Southworth
John Southworth*
Affiliation:
Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK email: [email protected]
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Abstract

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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.

Keywords

stars: binaries: eclipsingstars: oscillationsstars: fundamental parameters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 628 - 635
Copyright
Copyright © International Astronomical Union 2016 

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