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Pulsating variables from the OGLE and Araucaria projects
Published online by Cambridge University Press: 18 February 2014
Abstract
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