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Pulsating variables from the OGLE and Araucaria projects

Published online by Cambridge University Press:  18 February 2014

G. Pietrzyński
G. Pietrzyński*
Affiliation:
Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland email: [email protected] Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Chile
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Abstract

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We present some results of long-term studies of pulsating stars conducted in the course of the OGLE and Araucaria projects. In particular, very scarce eclipsing binaries containing pulsating stars are discussed. Such systems provide a unique opportunity to improve calibration of the cosmic distance scale and to better calibrate stellar evolutionary models.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 27 - 30
Copyright
Copyright © International Astronomical Union 2014 

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